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STAR FORMATION PowerPoint PPT Presentation
STAR FORMATION - typical densities above 1000 cm-3 ... PROTOSTARS: Emitting much IR radiation from infalling matter, usually in a flattened disk ...
typical densities above 1000 cm-3 ... PROTOSTARS: Emitting much IR radiation from infalling matter, usually in a flattened disk ...
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Simulating the Production of ICL in Galaxy Groups and Clusters PowerPoint PPT Presentation
Simulating the Production of ICL in Galaxy Groups and Clusters - Adaptive 2-D Gaussian smoothing kernel on each particle ... Luminosity shifts to higher surface brightness as groups infall. Huge ICL production after event ...
Adaptive 2-D Gaussian smoothing kernel on each particle ... Luminosity shifts to higher surface brightness as groups infall. Huge ICL production after event ...
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2MASS Image PowerPoint PPT Presentation
2MASS Image - LMSF region: Taurus. GMCs: Orion 'Intermediate': Ophiuchus 'Thermal' vs.'Turbulent' Cores ... Ammonia cores: 0.05pc, 10K, almost thermal support, sign of infall ...
LMSF region: Taurus. GMCs: Orion 'Intermediate': Ophiuchus 'Thermal' vs.'Turbulent' Cores ... Ammonia cores: 0.05pc, 10K, almost thermal support, sign of infall ...
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The%20Tension%20in%20Standard%20Big%20Bang%20Nucleosynthesis:%20Deuterium,%20Helium,%20Lithium%20and%20the%20Baryon%20Density PowerPoint PPT Presentation
The%20Tension%20in%20Standard%20Big%20Bang%20Nucleosynthesis:%20Deuterium,%20Helium,%20Lithium%20and%20the%20Baryon%20Density - David Tytler, David Kirkman, Nao Suzuki, Dan Lubin, Xiao-Ming Fan, Scott Burles, ... Depends on fraction of gas in stars, IMF, infall of gas with primordial D/H ...
David Tytler, David Kirkman, Nao Suzuki, Dan Lubin, Xiao-Ming Fan, Scott Burles, ... Depends on fraction of gas in stars, IMF, infall of gas with primordial D/H ...
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Dark Matter and Galaxy Formation Section 3: Galaxy Data vs' Simulations PowerPoint PPT Presentation
Dark Matter and Galaxy Formation Section 3: Galaxy Data vs' Simulations - Dark Matter and Galaxy Formation (Section 3: Galaxy Data vs. Simulations) Joel R. Primack ... Creation of halos and the infall of baryonic matter ...
Dark Matter and Galaxy Formation (Section 3: Galaxy Data vs. Simulations) Joel R. Primack ... Creation of halos and the infall of baryonic matter ...
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Astronomy and Astrophysics at SAO PowerPoint PPT Presentation
Astronomy and Astrophysics at SAO - From dust bunnies grow planets? Lee Hartmann, Smithonian Astrophysical Observatory. Protostars: images of (rotating) infall forming rotating disks. T Tauri disks ...
From dust bunnies grow planets? Lee Hartmann, Smithonian Astrophysical Observatory. Protostars: images of (rotating) infall forming rotating disks. T Tauri disks ...
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Galaxy Formation Theory II: Disk Galaxy Formation or What does the gas do when it gets there PowerPoint PPT Presentation
Galaxy Formation Theory II: Disk Galaxy Formation or What does the gas do when it gets there - Typical galaxy properties from simple arguments comparing tcool, tdyn, thubble. ... Infall. from. IGM. disk. Rvir. Rcool. MMW Formulae. Spin parameter ...
Typical galaxy properties from simple arguments comparing tcool, tdyn, thubble. ... Infall. from. IGM. disk. Rvir. Rcool. MMW Formulae. Spin parameter ...
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Evolution of the Earth PowerPoint PPT Presentation
Evolution of the Earth - Evolution of the Earth David Spergel Evolution of Earth s Atmosphere Earth lost its early atmosphere in major collisions (first 10-100 Myr) Subsequent infall of ...
Evolution of the Earth David Spergel Evolution of Earth s Atmosphere Earth lost its early atmosphere in major collisions (first 10-100 Myr) Subsequent infall of ...
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Gravitationally Unstable Protoplanetary Disks PowerPoint PPT Presentation
Gravitationally Unstable Protoplanetary Disks - dust emission with a scale of 100-400 AU. Outer radius ... Calvet et al. (1994) showed SEDs can be explained by dust emission from an infalling envelope ...
dust emission with a scale of 100-400 AU. Outer radius ... Calvet et al. (1994) showed SEDs can be explained by dust emission from an infalling envelope ...
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BAR FORMATION IN COSMOLOGICAL FRAMEWORK PowerPoint PPT Presentation
BAR FORMATION IN COSMOLOGICAL FRAMEWORK - Relaxed halo unrelaxed halo ( Curir Mazzei 99, 01) HOW THE DISK IS REACTING ... infall, the influence of the Dark Matter structure (triaxiality, substructure. ...
Relaxed halo unrelaxed halo ( Curir Mazzei 99, 01) HOW THE DISK IS REACTING ... infall, the influence of the Dark Matter structure (triaxiality, substructure. ...
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The origin of star formation at z 1: secular or episodic PowerPoint PPT Presentation
The origin of star formation at z 1: secular or episodic - LIRGs are witnessing the major morphological changes. Merger (minor & major), gas infall related to galaxy interaction, ... aligned with the disk major axis. ...
LIRGs are witnessing the major morphological changes. Merger (minor & major), gas infall related to galaxy interaction, ... aligned with the disk major axis. ...
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Galaxies in Clusters to z1 PowerPoint PPT Presentation
Galaxies in Clusters to z1 - H. Hoekstra (Leiden),), T. Webb (McGill) Rebin Yan (Toronto), K. ... Blue galaxies in clusters are generally consistent with an infalling coeval field population ...
H. Hoekstra (Leiden),), T. Webb (McGill) Rebin Yan (Toronto), K. ... Blue galaxies in clusters are generally consistent with an infalling coeval field population ...
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Correlation function in z and real space and consequences PowerPoint PPT Presentation
Correlation function in z and real space and consequences - Correlation function in z and real space and consequences. A MEASURE OF ... The nonlinear spherical infall model is then examined for cold-dark-matter power ...
Correlation function in z and real space and consequences. A MEASURE OF ... The nonlinear spherical infall model is then examined for cold-dark-matter power ...
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Model Chemical Evolution: PowerPoint PPT Presentation
Model Chemical Evolution: - Model Chemical Evolution: Starburst Environment. Once upon a time... Starburst environment, chemical evolution plays an important role. ...
Model Chemical Evolution: Starburst Environment. Once upon a time... Starburst environment, chemical evolution plays an important role. ...
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Black%20Hole%20Evaporation,%20Unitarity,%20and%20Final%20State%20Projection PowerPoint PPT Presentation
Black%20Hole%20Evaporation,%20Unitarity,%20and%20Final%20State%20Projection - Black Hole Evaporation, Unitarity, and Final State Projection Daniel Gottesman Perimeter Institute Black Hole Evaporation Information Loss Problem Solution 1 ...
Black Hole Evaporation, Unitarity, and Final State Projection Daniel Gottesman Perimeter Institute Black Hole Evaporation Information Loss Problem Solution 1 ...
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High-mass vs low-mass: the dividing line PowerPoint PPT Presentation
High-mass vs low-mass: the dividing line - High-mass vs low-mass: the dividing line ... precession of outflow complicate interpretation (Shepherd et al. 2000; Gibb et al. 2003) ...
High-mass vs low-mass: the dividing line ... precession of outflow complicate interpretation (Shepherd et al. 2000; Gibb et al. 2003) ...
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The Chemical and Color Evolution of M33 PowerPoint PPT Presentation
The Chemical and Color Evolution of M33 - rd,tot=2.4kpc, rd,*~1.4kpc. no merger. whole. gas & SFR. abundance. SB, color. Observation. H2,tot=0.2 109M, HItot=2.2 109M. rd,H2=2.5kpc, rd,tot=7.8kpc. whole ...
rd,tot=2.4kpc, rd,*~1.4kpc. no merger. whole. gas & SFR. abundance. SB, color. Observation. H2,tot=0.2 109M, HItot=2.2 109M. rd,H2=2.5kpc, rd,tot=7.8kpc. whole ...
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SMA Observations of the HH 212 Protostellar System Chin-Fei Lee, Paul P.T. Ho, Naomi Hirano, Henrik Beuther, Tyler L. Bourke, Hsien Shang, PowerPoint PPT Presentation
SMA Observations of the HH 212 Protostellar System Chin-Fei Lee, Paul P.T. Ho, Naomi Hirano, Henrik Beuther, Tyler L. Bourke, Hsien Shang, - a) A flattened envelope is seen in C18O (J=2-1) (red image) surrounding the ... supported (accretion) disk is expected to form within the envelope at ~ 70 AU. ...
a) A flattened envelope is seen in C18O (J=2-1) (red image) surrounding the ... supported (accretion) disk is expected to form within the envelope at ~ 70 AU. ...
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Ages, Metallicities and Abundances of Dwarf Early-Type Galaxies in the Coma Cluster by Ana Matkovic (STScI) PowerPoint PPT Presentation
Ages, Metallicities and Abundances of Dwarf Early-Type Galaxies in the Coma Cluster by Ana Matkovic (STScI) - Overall good agreement with NOAO Fundamental Plane Survey ( ); (Smith et al. 2005) ... Center galaxies with 100 kim/s. Center with 50 100 km/s. Center with ...
Overall good agreement with NOAO Fundamental Plane Survey ( ); (Smith et al. 2005) ... Center galaxies with 100 kim/s. Center with 50 100 km/s. Center with ...
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Young Stars I,II PowerPoint PPT Presentation
Young Stars I,II - Title: Star formation - the accretion (luminosity) problem Author: Lee Hartmann Last modified by: Lee Hartmann Created Date: 6/6/1999 2:12:30 PM Document presentation ...
Title: Star formation - the accretion (luminosity) problem Author: Lee Hartmann Last modified by: Lee Hartmann Created Date: 6/6/1999 2:12:30 PM Document presentation ...
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PowerPoint-Pr PowerPoint PPT Presentation
PowerPoint-Pr - gravitational torques (Hoyle 49; Peebles 69). High-resolution simulations find no ... Minor mergers don t change. or even decrease (d Onghia & Burkert, astro ...
gravitational torques (Hoyle 49; Peebles 69). High-resolution simulations find no ... Minor mergers don t change. or even decrease (d Onghia & Burkert, astro ...
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The formation of stars and planets PowerPoint PPT Presentation
The formation of stars and planets - The no support'-signal travels outward with sound speed ('expansion wave' ... Focal point of ellipse/parabola: Equator. r. rm. re. a. vm. Ang. Mom. Conserv: ...
The no support'-signal travels outward with sound speed ('expansion wave' ... Focal point of ellipse/parabola: Equator. r. rm. re. a. vm. Ang. Mom. Conserv: ...
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Gas in the Local Group PowerPoint PPT Presentation
Gas in the Local Group - Gas in the Local Group
Gas in the Local Group
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Mitch Begelman PowerPoint PPT Presentation
Mitch Begelman - Mitch Begelman. JILA, University of Colorado. FORMATION AND ... YOU'VE GOT TO BE KIDDING. QUASISTAR PROPERTIES. Mass m* (M ) increases with time. Core with ...
Mitch Begelman. JILA, University of Colorado. FORMATION AND ... YOU'VE GOT TO BE KIDDING. QUASISTAR PROPERTIES. Mass m* (M ) increases with time. Core with ...
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LoCuSS: The midinfrared ButcherOemler effect Chris Haines University of Birmingham LoCuSS: Graham Sm PowerPoint PPT Presentation
LoCuSS: The midinfrared ButcherOemler effect Chris Haines University of Birmingham LoCuSS: Graham Sm - LoCuSS: The midinfrared ButcherOemler effect Chris Haines University of Birmingham LoCuSS: Graham Sm
LoCuSS: The midinfrared ButcherOemler effect Chris Haines University of Birmingham LoCuSS: Graham Sm
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The Star Formation- Density Relation PowerPoint PPT Presentation
The Star Formation- Density Relation - Age-density relation for ageing (E-Sb) galaxies ... Galaxy transformation during plenty of ... Dusty red galaxies in A901. are semi-suppressed in star formation ...
Age-density relation for ageing (E-Sb) galaxies ... Galaxy transformation during plenty of ... Dusty red galaxies in A901. are semi-suppressed in star formation ...
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Thermalization of Gauge Theory and Gravitational Collapse PowerPoint PPT Presentation
Thermalization of Gauge Theory and Gravitational Collapse - In large Nc, strong coupling limit, string theory in AdS5xS5 background is dual to N=4 SYM ... hologram of the debris. Q. Qbar. SL, E.Shuryak arXiv:0711.0736 [hep-th] ...
In large Nc, strong coupling limit, string theory in AdS5xS5 background is dual to N=4 SYM ... hologram of the debris. Q. Qbar. SL, E.Shuryak arXiv:0711.0736 [hep-th] ...
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AdSCFT Applications PowerPoint PPT Presentation
AdSCFT Applications - Heavy Quark with v 1 neglect radiation. HQ classical on medium correlations scale ... Add an external electric field to valance the drag. v. Einstein relations ...
Heavy Quark with v 1 neglect radiation. HQ classical on medium correlations scale ... Add an external electric field to valance the drag. v. Einstein relations ...
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The Rocket Science of Launching Stellar Disks PowerPoint PPT Presentation
The Rocket Science of Launching Stellar Disks - Where do stars, planets, we, come from?? From collapse of ... Spiral Galaxies. Disk in Center of Galaxy. Beta Pictoris. Lagoon. Nebula. Gaseous Pillars in M16 ...
Where do stars, planets, we, come from?? From collapse of ... Spiral Galaxies. Disk in Center of Galaxy. Beta Pictoris. Lagoon. Nebula. Gaseous Pillars in M16 ...
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Theoretical Motivation for Submm-VLBI of Sgr A* PowerPoint PPT Presentation
Theoretical Motivation for Submm-VLBI of Sgr A* - Dark matter particles: weakly interacting bosons and scalar fields may ... Can one form a central dark ... no solid surface ('boson sponge') and no horizon ...
Dark matter particles: weakly interacting bosons and scalar fields may ... Can one form a central dark ... no solid surface ('boson sponge') and no horizon ...
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Mitch Begelman PowerPoint PPT Presentation
Mitch Begelman - Mitch Begelman
Mitch Begelman
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Formation of Stars and Planets PowerPoint PPT Presentation
Formation of Stars and Planets - Formation of Stars and Planets Frank H. Shu National Tsing Hua University Arnold Lecture UC San Diego 6 May 2005 Outline of Talk Origin of solar system review ...
Formation of Stars and Planets Frank H. Shu National Tsing Hua University Arnold Lecture UC San Diego 6 May 2005 Outline of Talk Origin of solar system review ...
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Determination of physical properties from molecular lines Kate Brooks Australia Telescope National Facility PowerPoint PPT Presentation
Determination of physical properties from molecular lines Kate Brooks Australia Telescope National Facility - ... {7|7}7~77 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 ... WoXoYoo[oo]o^o_o`oaobocodoeofogohoiojokolomonooopoqorosotouovowoxoyozo{o|o }o~o ...
... {7|7}7~77 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 7 ... WoXoYoo[oo]o^o_o`oaobocodoeofogohoiojokolomonooopoqorosotouovowoxoyozo{o|o }o~o ...
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High%20Resolution%20Observations%20in%20B1-IRS: PowerPoint PPT Presentation
High%20Resolution%20Observations%20in%20B1-IRS: - High Resolution Observations in B1-IRS: ammonia , CCS and water masers. Claire Chandler, NRAO ... dynamics and evolution at high resolution. - Test CCS vs NH3 ...
High Resolution Observations in B1-IRS: ammonia , CCS and water masers. Claire Chandler, NRAO ... dynamics and evolution at high resolution. - Test CCS vs NH3 ...
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AdSCFT and transport constants in Expanding QGP PowerPoint PPT Presentation
AdSCFT and transport constants in Expanding QGP - ... gravity duality. D-brane AdS ... in the frame following a particle. Boundary. Horizon. Equation of Motion ... Normalization of wave function. Result ...
... gravity duality. D-brane AdS ... in the frame following a particle. Boundary. Horizon. Equation of Motion ... Normalization of wave function. Result ...
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STUDIO DI PowerPoint PPT Presentation
STUDIO DI - STUDIO DI STAR FORMATION HISTORY DA SPETTRI COSMICI Martinelli Federica Seminario finale per il corso di COSMOLOGIA OSSERVATIVA Prof. Guido Chincarini
STUDIO DI STAR FORMATION HISTORY DA SPETTRI COSMICI Martinelli Federica Seminario finale per il corso di COSMOLOGIA OSSERVATIVA Prof. Guido Chincarini
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AdSCFT Calculations of Parton Energy Loss PowerPoint PPT Presentation
AdSCFT Calculations of Parton Energy Loss - The QGP at T=(1-2)Tc may be strongly coupled: ... Add an external electric field to valance the drag. v. 10. Broadening of a Fast Probe ...
The QGP at T=(1-2)Tc may be strongly coupled: ... Add an external electric field to valance the drag. v. 10. Broadening of a Fast Probe ...
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Galaxy Growth: The role of environment PowerPoint PPT Presentation
Galaxy Growth: The role of environment - Anna Pasquali, Dan McIntosh, Xiaohu Yang, Houjun Mo ... No major rearrangement. of mass distribution. by environmental process - evidence against ...
Anna Pasquali, Dan McIntosh, Xiaohu Yang, Houjun Mo ... No major rearrangement. of mass distribution. by environmental process - evidence against ...
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Momentum Broadening of Heavy Probes in Strongly Couple Plasmas PowerPoint PPT Presentation
Momentum Broadening of Heavy Probes in Strongly Couple Plasmas - Close to V=0 both behave as v=0 case same analyticity continuation ... world sheet horizon we impose the same analyticity condition as for in the v=0 case. ...
Close to V=0 both behave as v=0 case same analyticity continuation ... world sheet horizon we impose the same analyticity condition as for in the v=0 case. ...
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Surveys of high-z galaxies and galaxy clusters with Herschel and SCUBA-2 PowerPoint PPT Presentation
Surveys of high-z galaxies and galaxy clusters with Herschel and SCUBA-2 - H1K fields (white blocks) superimposed on the IRAS 100 micron maps ... A blank field (850 micron @ JCMT) Add a (proto-)cluster at z=2.5 ...
H1K fields (white blocks) superimposed on the IRAS 100 micron maps ... A blank field (850 micron @ JCMT) Add a (proto-)cluster at z=2.5 ...
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Extended%20ionized%20gas%20regions%20around%20the%20Coma%20cluster%20galaxies PowerPoint PPT Presentation
Extended%20ionized%20gas%20regions%20around%20the%20Coma%20cluster%20galaxies - Extended ionized gas regions around the Coma cluster galaxies Michitoshi YOSHIDA Okayama Astrophysical Observatory, NAOJ with Masafumi Yagi, Sadanori Okamura, Yutaka ...
Extended ionized gas regions around the Coma cluster galaxies Michitoshi YOSHIDA Okayama Astrophysical Observatory, NAOJ with Masafumi Yagi, Sadanori Okamura, Yutaka ...
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Black Holes: Spacetime vs. Quantum Mechanics PowerPoint PPT Presentation
Black Holes: Spacetime vs. Quantum Mechanics - Black Holes: Spacetime vs. Quantum Mechanics Joseph Polchinski CCGRRA, Winnipeg, 5/21/14
Black Holes: Spacetime vs. Quantum Mechanics Joseph Polchinski CCGRRA, Winnipeg, 5/21/14
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Extraplanar HI and its implications PowerPoint PPT Presentation
Extraplanar HI and its implications - Extraplanar HI and its implications
Extraplanar HI and its implications
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Chemistry in low-mass star forming regions: ALMA PowerPoint PPT Presentation
Chemistry in low-mass star forming regions: ALMA - Title: PowerPoint Presentation Last modified by: Created Date: 1/1/1601 12:00:00 AM Document presentation format:
Title: PowerPoint Presentation Last modified by: Created Date: 1/1/1601 12:00:00 AM Document presentation format:
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SUMMARY PowerPoint PPT Presentation
SUMMARY - SUMMARY Statistical equilibrium and radiative transfer in molecular (H2) cloud Derivation of physical parameters of molecular clouds High-mass star formation ...
SUMMARY Statistical equilibrium and radiative transfer in molecular (H2) cloud Derivation of physical parameters of molecular clouds High-mass star formation ...
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High Resolution 4'7 m KeckNIRSPEC Spectra of Protostars PowerPoint PPT Presentation
High Resolution 4'7 m KeckNIRSPEC Spectra of Protostars - High Resolution 4.7 m Keck/NIRSPEC Spectra of Protostars. R=25,000 in 0.43' wide ... cannot observe sources without optical guide star closeby (4 arcmin), i.e. ...
High Resolution 4.7 m Keck/NIRSPEC Spectra of Protostars. R=25,000 in 0.43' wide ... cannot observe sources without optical guide star closeby (4 arcmin), i.e. ...
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From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation PowerPoint PPT Presentation
From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation - From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ed. V ...
From Pre-Stellar Cores to Protostars: The Initial Conditions of Star Formation Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ed. V ...
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Outflow interaction at late stages of star formation PowerPoint PPT Presentation
Outflow interaction at late stages of star formation - ... 1 1111 ... T. O. d. f. e. n. * P ''a GpSs tFTOdfe n ...
... 1 1111 ... T. O. d. f. e. n. * P ''a GpSs tFTOdfe n ...
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Young Stars I,II PowerPoint PPT Presentation
Young Stars I,II - Essentially ALL protostellar cloud magnetic flux must be lost during star ... collimation. Alfven surface. Accretion leads to ejection. dM/dt (wind) = 0.1 dM/dt (acc) ...
Essentially ALL protostellar cloud magnetic flux must be lost during star ... collimation. Alfven surface. Accretion leads to ejection. dM/dt (wind) = 0.1 dM/dt (acc) ...
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The Location and Kinematics PowerPoint PPT Presentation
The Location and Kinematics - Future Directions in High Resolution Astronomy: A Celebration of the 10th ... J.E. Conway, G.K. Miley, C.P. O'Dea, H.J.A. R ttgering, ...
Future Directions in High Resolution Astronomy: A Celebration of the 10th ... J.E. Conway, G.K. Miley, C.P. O'Dea, H.J.A. R ttgering, ...
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Chemical Evolution of the Milky Way PowerPoint PPT Presentation
Chemical Evolution of the Milky Way - Mass to light ratios vs. Galaxy absolute V magnitude (Gilmore et al. 2006) ... Carigi, Hernandez & Gilmore (2002) computed models for 4 dSphs by assuming SF ...
Mass to light ratios vs. Galaxy absolute V magnitude (Gilmore et al. 2006) ... Carigi, Hernandez & Gilmore (2002) computed models for 4 dSphs by assuming SF ...
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Extended ionized gas regions around the Coma cluster galaxies PowerPoint PPT Presentation
Extended ionized gas regions around the Coma cluster galaxies - inter-galactic features in these data. Extended Ionized. Gas around the. Coma galaxies ... RB199: Splash-like filaments star-formation in the inter-galactic space ...
inter-galactic features in these data. Extended Ionized. Gas around the. Coma galaxies ... RB199: Splash-like filaments star-formation in the inter-galactic space ...
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Galaxy-to IGM feedback of magnetic energy and implications for UHECR PowerPoint PPT Presentation
Galaxy-to IGM feedback of magnetic energy and implications for UHECR - Galaxyto IGM feedback of magnetic energy and implications for UHECRs
Galaxyto IGM feedback of magnetic energy and implications for UHECRs
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Two ways for mass assembly of galaxies PowerPoint PPT Presentation
Two ways for mass assembly of galaxies - The abundance of massive galaxies at high z is compatible with models. 6 ... (E A, or k a), with no current star formation but strong Balmer abs ...
The abundance of massive galaxies at high z is compatible with models. 6 ... (E A, or k a), with no current star formation but strong Balmer abs ...
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From PreStellar Cores to Protostars: The Initial Conditions of Star Formation PowerPoint PPT Presentation
From PreStellar Cores to Protostars: The Initial Conditions of Star Formation - Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ... Introduction: Stages of low-mass ... SCUBA on JCMT (submm) IRAM (mm) 10/18/09 ...
Andre P., Ward-Thompson D., Barsony M., 2000, in Protostars and Planets IV, ... Introduction: Stages of low-mass ... SCUBA on JCMT (submm) IRAM (mm) 10/18/09 ...
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How do Galaxies Get Their Gas PowerPoint PPT Presentation
How do Galaxies Get Their Gas - Why is SFR density so high at early times and decreases at low-z? ... Amount of gas in DLA at high-z is less than the mass locked in stars at z=0. ...
Why is SFR density so high at early times and decreases at low-z? ... Amount of gas in DLA at high-z is less than the mass locked in stars at z=0. ...
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