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1.Astronomy & Astrophysics manuscript no. SSLep-final ⃝ ESO 2011c November 28, 2011An incisive look at the symbiotic star SS Leporis⋆ Milli-arcsecond imaging with…

Documents Ammonia and CCS as diagnostic tools of low-mass protostars Ammonia and CCS as diagnostic tools of...

Slide 1 Ammonia and CCS as diagnostic tools of low-mass protostars Ammonia and CCS as diagnostic tools of low-mass protostars Itziar de Gregorio-Monsalvo (ESO /ALMA fellow…

Documents Ammonia and CCS as diagnostic tools of low-mass protostars

Ammonia and CCS as diagnostic tools of low-mass protostars Itziar de Gregorio-Monsalvo (ESO /ALMA fellow in Chile) Collaborators: J.F. Gómez (IAA, Spain) C.J. Chandler (NRAO,…

Documents Big World of Small Neutrinos

Big World of Small Neutrinos Roman Shcherbakov 21, March, 2007 3 Nobel prizes 1988 LEDERMAN, SCHWARTZ and JACK STEINBERGER â detected muon neutrinos 1995 REINES â detected…

Documents Intermittent Accreting Millisecond Pulsars

Intermittent Accreting Millisecond Pulsars Introduction An exciting new type of sources Pulsations appear and disappear either on timescales of hundreds of seconds or on…

Documents Discovery of IRC10216 Eric Becklin Offscale. IRC+10216 Old carbon rich red giant with a dusty...

Discovery of IRC10216 Eric Becklin Offscale IRC+10216 Old carbon rich red giant with a dusty expanding shell at 10-20 km s-1 Harry Kroto 2004 Harry Kroto 2004 Central warm…

Documents Type Ia Supernova Explosion Mechanisms or How to Blow Up a White Dwarf Jeffrey M. Silverman Astro...

Type Ia Supernova Explosion Mechanisms or How to Blow Up a White Dwarf Jeffrey M. Silverman Astro 254: HEAp 5/1/2006 What are Type Ia Supernovae? White Dwarf (WD): an evolved…

Documents COS Observations of the Chemical Composition of SNR LMC N132D France et al. Ben Folsom and Sharlene....

COS Observations of the Chemical Composition of SNR LMC N132D France et al. Ben Folsom and Sharlene Rubio Background on Supernovae: -Fe56 is the most stable isotope inside…

Documents COS Observations of the Chemical Composition of SNR LMC N132D France et al.

COS Observations of the Chemical Composition of SNR LMC N132D France et al. Ben Folsom and Sharlene Rubio Background on Supernovae: -Fe56 is the most stable isotope inside…

Documents The life of stars

The life of stars The life of stars The Interstellar Medium What is a light year? How many miles in a light year? Why is it called a light year? Just how fast is light? Constellation…