'Massive black holes' diaporamas de présentation

OH Megamaser Studies at Arecibo: Current Studies and Future Directions

OH Megamaser Studies at Arecibo: Current Studies and Future Directions. Jeremy Darling (Carnegie Observatories). Collaborators: Riccardo Giovanelli (Cornell) Ylva Pihlstroem (NRAO) James Cordes (Cornell) Karl Menten (MPIFR) Alison Peck (CfA).

491 views • 33 slides

Joan Centrella Gravitational Astrophysics Laboratory NASA/GSFC

494 views • 29 slides

Joan Centrella Gravitational Astrophysics Laboratory NASA/GSFC

466 views • 29 slides

Quasars and Massive Black Holes

Quasars and Massive Black Holes. Stephen Fine. Outline. What is a quasar How do we study quasar black holes Why do we study quasar black holes What are the current difficulties in studying black holes How can we improve on the current situation. What is a quasar?. This is not a quasar.

382 views • 21 slides

FRI RADIO GALAXIES AT z > 1 STUDYING THE BUILDING BLOCKS OF

FRI RADIO GALAXIES AT z > 1 STUDYING THE BUILDING BLOCKS OF TODAY'S MOST MASSIVE GALAXIES AND CLUSTERS Marco Chiaberge Space Telescope Science Institute and INAF-IRA Bologna G. Tremblay (STScI) A. Capetti (INAF-OATO) D. Macchetto (STScI) W.B. Sparks (STScI) P. Tozzi (INAF-OATS).

282 views • 16 slides

Unit 2 Seminar

Unit 2 Seminar. SC300 Eric Bliss. Black Holes: What Are They?. Black holes are the evolutionary endpoints of stars at least 10 to 15 times as massive as the Sun. If a star that massive undergoes a supernova explosion, it may leave behind a fairly massive burned out stellar remnant.

296 views • 15 slides

GSMT NSF Science Working Group

GSMT NSF Science Working Group. Rolf-Peter Kudritzki NOAO Town Meeting 07 January, 2003. Goals of the SWG. SWG is a community-based group convened to: Formulate an inspiring and powerful science case for federal investment in GSMT Identify key science drivers

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Black Holes

Black Holes. Chapter 14. Review. What is the life cycle of a low mass star (<8 solar masses when on the main sequence)? What is the life cycle of a high mass star (>8 solar masses when on the main sequence)? After a supernova, what are the two fates of the core of the star?

180 views • 12 slides