Radioquiet PowerPoint PPT Presentations

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RadioLoud and RadioQuiet, Gammaray Pulsars from the Galaxy and the Gould Belt PowerPoint PPT Presentation

RadioLoud and RadioQuiet, Gammaray Pulsars from the Galaxy and the Gould Belt - Radio beam geometry and velocity kick distribution Arzoumanian, Chernoff & Cordes (2002) ... to 978 radio pulsars (Galactic plane) to 120 supernovae in the Gould Belt ...

Radio beam geometry and velocity kick distribution Arzoumanian, Chernoff & Cordes (2002) ... to 978 radio pulsars (Galactic plane) to 120 supernovae in the Gould Belt ...

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Did I say radio quiet Radioloudness in radioquiet Seyferts and a note on Xray core spectra in lowpow PowerPoint PPT Presentation

Did I say radio quiet Radioloudness in radioquiet Seyferts and a note on Xray core spectra in lowpow - Gallery of radio emission in Seyferts. Unresolved. Sub-pc scale. 0.1 pc. NGC4395 ... Sources with ionization cones host larger radio sources ...

Gallery of radio emission in Seyferts. Unresolved. Sub-pc scale. 0.1 pc. NGC4395 ... Sources with ionization cones host larger radio sources ...

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Close-by young isolated neutron stars (and black holes) PowerPoint PPT Presentation

Close-by young isolated neutron stars (and black holes) - Close-by young isolated neutron stars (and black holes) Sergey Popov (Sternberg Astronomical Institute) Plan of the talk NS: introduction Close-by NSs Population ...

Close-by young isolated neutron stars (and black holes) Sergey Popov (Sternberg Astronomical Institute) Plan of the talk NS: introduction Close-by NSs Population ...

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Lecture 1 Isolated Neutron Stars. Intro. PowerPoint PPT Presentation

Lecture 1 Isolated Neutron Stars. Intro. - Neutron stars have been predicted in 30s: L.D. Landau: Star-nuclei (1932) anecdote ... (Landau) (Baade) (Zwicky) 4. Good old classics. The pulsar in the Crab ...

Neutron stars have been predicted in 30s: L.D. Landau: Star-nuclei (1932) anecdote ... (Landau) (Baade) (Zwicky) 4. Good old classics. The pulsar in the Crab ...

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Solar vicinity, close-by young isolated NSs, and tests of cooling curves PowerPoint PPT Presentation

Solar vicinity, close-by young isolated NSs, and tests of cooling curves - Solar vicinity, close-by young isolated NSs, and tests of cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke

Solar vicinity, close-by young isolated NSs, and tests of cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke

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Lecture 1 Isolated Neutron Stars. Intro. PowerPoint PPT Presentation

Lecture 1 Isolated Neutron Stars. Intro. - Recent data Calvera et al. LOFAR Gravitational waves from INSs Recent LIGO results for PSRs GWs from young magnetars Detectability by advanced LIGO Magnetar ...

Recent data Calvera et al. LOFAR Gravitational waves from INSs Recent LIGO results for PSRs GWs from young magnetars Detectability by advanced LIGO Magnetar ...

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Isolated Neutron Stars. Intro. PowerPoint PPT Presentation

Isolated Neutron Stars. Intro. - Isolated Neutron Stars. Intro. Stars in the Galaxy Prediction ... Good old classics The old zoo of neutron stars Rocket experiments Sco X-1 UHURU Accretion in close ...

Isolated Neutron Stars. Intro. Stars in the Galaxy Prediction ... Good old classics The old zoo of neutron stars Rocket experiments Sco X-1 UHURU Accretion in close ...

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Isolated Neutron Stars. Intro. PowerPoint PPT Presentation

Isolated Neutron Stars. Intro. - Stars in the Galaxy Prediction ... (single template) 2. 0708.3818 All-sky search for periodic grav. waves in LIGO S4 data 50-1000 HZ No evidence.

Stars in the Galaxy Prediction ... (single template) 2. 0708.3818 All-sky search for periodic grav. waves in LIGO S4 data 50-1000 HZ No evidence.

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Close-by young isolated neutron stars (and black holes) PowerPoint PPT Presentation

Close-by young isolated neutron stars (and black holes) - Close-by young isolated neutron stars (and black holes) Sergey Popov (Sternberg Astronomical Institute) Plan of the talk NS: introduction Close-by NSs Population ...

Close-by young isolated neutron stars (and black holes) Sergey Popov (Sternberg Astronomical Institute) Plan of the talk NS: introduction Close-by NSs Population ...

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Close-by young isolated NSs: A new test for cooling curves PowerPoint PPT Presentation

Close-by young isolated NSs: A new test for cooling curves - Close-by young isolated NSs: A new test for cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke

Close-by young isolated NSs: A new test for cooling curves Sergei Popov (Sternberg Astronomical Institute) Co-authors: H.Grigorian, R. Turolla, D. Blaschke

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Evolution%20of%20isolated%20neutron%20stars:%20young%20coolers%20and%20old%20accretors PowerPoint PPT Presentation

Evolution%20of%20isolated%20neutron%20stars:%20young%20coolers%20and%20old%20accretors - Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...

Evolution of isolated neutron stars: young coolers and old accretors Sergei Popov (SAI) Plan of the talk Magnetic rotator Evolution of neutron stars: rotation ...

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Space%20Cowboys%20Odissey:%20Beyond%20the%20Gould%20Belt PowerPoint PPT Presentation

Space%20Cowboys%20Odissey:%20Beyond%20the%20Gould%20Belt - Title: Close-by young isolated neutron stars (and black holes) Author: polar Last modified by: sergepolar Created Date: 4/1/2005 6:24:30 AM Document presentation format

Title: Close-by young isolated neutron stars (and black holes) Author: polar Last modified by: sergepolar Created Date: 4/1/2005 6:24:30 AM Document presentation format

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Neutron star masses: dwarfs, giants and neighbors PowerPoint PPT Presentation

Neutron star masses: dwarfs, giants and neighbors - Neighbors: young and slim. Initial NS mass spectrum is unknown ... Young close-by NSs are slim 1.4Msun. Mass constraint can be useful for ...

Neighbors: young and slim. Initial NS mass spectrum is unknown ... Young close-by NSs are slim 1.4Msun. Mass constraint can be useful for ...

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Isolated Neutron Stars. Intro. PowerPoint PPT Presentation

Isolated Neutron Stars. Intro. - Stars in the Galaxy Prediction ... (single template) 2. 0708.3818 All-sky search for periodic grav. waves in LIGO S4 data 50-1000 HZ No evidence.

Stars in the Galaxy Prediction ... (single template) 2. 0708.3818 All-sky search for periodic grav. waves in LIGO S4 data 50-1000 HZ No evidence.

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Isolated Neutron Stars and Black Holes. Intro. PowerPoint PPT Presentation

Isolated Neutron Stars and Black Holes. Intro. - Isolated Neutron Stars and Black Holes. Intro. Sergei Popov (SAI MSU) Plan Part 1. Neutron stars Prediction ... Good old classics The old zoo of neutron stars Rocket ...

Isolated Neutron Stars and Black Holes. Intro. Sergei Popov (SAI MSU) Plan Part 1. Neutron stars Prediction ... Good old classics The old zoo of neutron stars Rocket ...

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Solar vicinity, closeby young isolated NSs, and tests of cooling curves PowerPoint PPT Presentation

Solar vicinity, closeby young isolated NSs, and tests of cooling curves - Later on: six brothers. RX J1856.5-3754. 5. Magnificent Seven. 9.44 ... in the low-frequency band (60-110 MHz) with the radio telescope in Pushchino. (back) ...

Later on: six brothers. RX J1856.5-3754. 5. Magnificent Seven. 9.44 ... in the low-frequency band (60-110 MHz) with the radio telescope in Pushchino. (back) ...

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The Zoo Of Neutron Stars PowerPoint PPT Presentation

The Zoo Of Neutron Stars - Unidentified EGRET sources. Transient radio sources (RRATs) Calvera ... no radio pulsars in 56 EGRET error boxes (Crawford et al. 2006) ...

Unidentified EGRET sources. Transient radio sources (RRATs) Calvera ... no radio pulsars in 56 EGRET error boxes (Crawford et al. 2006) ...

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The IwasawaTaniguchi effect for radioquiet AGN PowerPoint PPT Presentation

The IwasawaTaniguchi effect for radioquiet AGN - Most of the iron line flux comes from the 'torus', not the BLR ... (Eddington ratio) of the covering factor of the torus (similar effect found in IR) ...

Most of the iron line flux comes from the 'torus', not the BLR ... (Eddington ratio) of the covering factor of the torus (similar effect found in IR) ...

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