Slide 1 Slide 2 Slide 3 §A. A polish astronomer in the 16th Century, realized that our model of our solar system worked much better if we put the Sun at the center and not…

Slide 1Formation of Stars and Galaxies Slide 2 Introduction 1.Timeline and Big Bang Slide 3 The Instruments 1. Optical Telescopes a)Use different regions of Electromagnetic…

Slide 1 The Deaths of Sunlike Stars Slide 2 Low Mass Dwarfs Low mass red dwarf stars cannot achieve any advanced fusion because they cannot get hot enough (Temp < 100…

Slide 1 Compact Objects Astronomy 315 Professor Lee Carkner Lecture 15 “How will we see when the sun goes dark?” “We will be forced to grope and feel our way.” --Jack…

Slide 1 Astronomy for beginners Black Holes Aashman Vyas Slide 2 What are Black Holes? A black hole is a super dense object that has an intense gravitational pull There are…

Forming Nonsingular Black Holes from Dust Collapse by R. Maier (Centro Brasileiro de Pesquisas Físicas-Rio de Janeiro) I. Damião Soares (Centro Brasileiro de Pesquisas…

Hawking Radiations and Anomalies Satoshi Iso (KEK) based on collaborations while I was staying at MIT(05/03-06/01) with Hiroshi Umetsu (OIQP) and Frank Wilczek (MIT) hep-th/0602146…

    Прецизионные измерения гравитационных возмущений оптическими интерферометрами с большой…

Relativistic Astrophysics: general overview Jean-Pierre Lasota Lecture 1 For a neutron star Po= 1.41 a (Haensel, Lasota & Zdunik 1999) (a = 2GM/c2) Einstein A, On a stationary…

TURN TO THE BACK PAGE FOR CALENDAR INFORMATION NewsletterNewsletterNewsletterNewsletter December 2010 Issue 2Issue 2Issue 2Issue 2 âAiming for ExcellenceâAiming for ExcellenceâAiming…