With help from many, including Andrzej Baran, Staszek Zola, ... Teff=29635 K (29,500 /-500) log g = 5.518 (5.50 /-0.05) Near core He exhaustion (0.74% by mass) ...
... population of faint blue blue stars in our galaxy and giant elliptical galaxies ... Early 1980's helium-rich and helium-poor objects thought to be separated by a ...
Evolution has been the subject of much debate although binary evolution is ... high mass loss on the red giant branch undergo a late helium core flash on the ...
24, June 2002. white dwarf mergers. The progeny of binary white dwarf mergers; ... Progeny of WD WD mergers ? Extreme Helium stars. RCrB stars. subdwarf B stars ...
white dwarf mergers. The progeny of binary white dwarf mergers; ... (Landau & Lifshitz 1958) CO He merger frequency: 4.4 10-3 yr-1 (Neleman's et al. 2001) ...
Variability discovered by Ostensen et al. (2001) Five frequencies ... Amplitudes between 0.3-10.2 mmag. Subdwarf sdB star. August 5-11, Moletai (165cm) 2004 ...
Carlos S nchez (TCS, 1.55 m) Big field OGS (1 m) Stare (10 cm) www.iac.es/ot ... Juan A. Belmonte. Sebasti n Jim nez. Hans Deeg. Lexter Fox (just PhD finished) ...
... (top right) is a 3-channel photometer, used for measuring starlight in three ... In 2005 May it was mounted on one unit of the ESO Very Large Telescope at ...
Brown Dwarf Science with VLST. Outline: The Big Questions. Where we are and how VLST would help... Brown Dwarf Science with VLST. 2MASS and SDSS find ...
Internal dynamics from asteroseismology for two sdB pulsators residing in close binary systems Val rie Van Grootel (Laboratoire d Astrophysique de Toulouse ...
and related objects Progress in the asteroseismic analysis of the pulsating sdB star PG 1605+072 Val rie Van Grootel (Laboratoire d Astrophysique de Toulouse, France)
... only from higher-excitation Si I yellow-red lines ... n-capture, recent lab transitions. Three groups contribute especially: Lund, Liege, Wisconsin ...
The (second) widest ultracool binary: a challenge for very low-mass formation ... The widest system containing an L dwarf component. Primary: HD 221356 (F8.0V; ...
To Be or Not to Be: The Mysteries of Disk Formation Around Rapidly Spinning Be Stars Douglas R. Gies Department of Physics and Astronomy Center for High Angular ...
Astroparticle physics. 1. stellar astrophysics and solar neutrinos. Alberto Carrami ana. Instituto Nacional de Astrof sica, ptica y Electr nica. Tonantzintla, ...
Jodrell Bank. Registry and DIS. High Volume Storage. Raid 5, 4 Terabyte ... Column: Representation of TD from VOTable. Parser Design. API Typical Operations ...
1- Pulsators in late stages of stellar evolution: their location ... reflexion of waves with nodes at transition zones. fractional mass above transition zones ...
A round or axisymmetric shape, sometimes with multiple shells or outer haloes. ... Silkworm. NGC 6302. Hb 5. Size does matter! 28. 28. A necessary question...
Extrasolar planets one of the major astronomical topic of the last decade ... Transit survey approved for GTO bright time on VST. PI: Snellen (Leiden Observatory) ...
D.Pollacco, QUB, R.Starling, MSSL, P.W.Hill, St Andrews University. based on work published in MNRAS 313, 671, MNRAS 321,111 and accepted by MNRAS and A&A ...
Stars WD, CV, BHB, BD etc. Serendipity. Rare populations found in SDSS ... 12 Ts and ~100 Ls. Fan et al. 2001. Fan, Narayanan, Strauss, Becker, White et al. z ...
Halo Velocity Dispersion. Old Disk. Velocity. Dispersion. Biases? 2s. 1s ... stellar halo should have 2 2.5 x 10-5 pc-3. But, what does this really mean? ...
DATA MODELS: This initiative aims to define the common elements of astronomical ... Federation and joining of information become possible and Grid computing is ...
detects even light cirrus under a full range of moon phases (no ... These assume that only two filters will be observed each night (either g and r, or i and z) ...
Definition of a star: a gravitationally-bound sphere of gas massive ... Jovian planets defined to be up to 13 MJ (0.013 M ) Brown dwarfs 0.013 - 0.075 M ...
Faint stars usually have no name. The Names of Sirius. Alpha Canis Majoris (Bayer, 1603) ... Examples: Vega, Sirius. The Main Sequence: F. Temperature: 6000 ...
... by treating cleveite with mineral acids. ... Cleveite is an impure ... cleveite. Pierre Jules. Janssen: 1824-1907. Lord Rutherford: 1871-1937. Helium ...
... Mead 1965, Press et al. 1989): uses a self-modifying cell (AMOEBA) that ' ... UV Flux distributions are often degenerate in EB-V and Teff (even the 2175 bump ...
... Search for Substellar Companions in the Halo of Nearby Stars ... Ls. Burrows et al. 1997. Searches for Brown Dwarfs. Companions to nearby stars. Direct Imaging ...
Picture of UV ionizing background. Difficulty in studying quasar evolution ... AGN activity in galaxy evolution picture, and the realization of the connection ...
thillwig@chara.gsu.edu. Abstract ... In both cases, the variability shows very little scatter from a sine curve. ... theory he classified a large number of PNe, ...
Rachel Osten (P): Detected variable 3.6 cm and 6 cm emission from the M8.5 V ... Ray Jayarardhana: Accreting brown dwarfs are slow rotators, so disk locking ...
12. Star Count Analysis (see Mihalas & Routly, Galactic Astronomy) Define, for a particular area of sky: N(m) = total number of stars brighter than magnitude m per ...
V652 Her: evidence that white dwarf mergers ... The British Council, the Japan Society for the Promotion of ... observationally distinguishable groups of ...