<--- Back to Details
First PageDocument Content
Stellar evolution / Star types / Asymptotic giant branch / Planetary nebula / Protoplanetary nebula / Supernova / Red supergiant / Infrared excess / White dwarf / Carbon star / Star formation / S-process
Date: 2012-05-01 04:50:26
Stellar evolution
Star types
Asymptotic giant branch
Planetary nebula
Protoplanetary nebula
Supernova
Red supergiant
Infrared excess
White dwarf
Carbon star
Star formation
S-process

Add to Reading List

Source URL: www.astro.keele.ac.uk

Download Document from Source Website

File Size: 157,39 KB

Share Document on Facebook

Similar Documents

Star Formation In Nearby “Extreme” Galaxies Yong Shi (施勇,Nanjing University) Collaborators: Lee Armus (Caltech, US), Yu Gao (PMO, China), Qiusheng Gu (NJU, China), George Helou (Caltech, US), Sabrina Stierwalt

DocID: 1vr9c - View Document

A The Astronomical Journal, 132:2539Y2555, 2006 December # 2006. The American Astronomical Society. All rights reserved. Printed in U.S.A. CLUES TO NUCLEAR STAR CLUSTER FORMATION FROM EDGE-ON SPIRALS

DocID: 1uWdf - View Document

Large scale MD simulations of nuclear pasta formation: Nuclear reactions that make a neutron star Objectives: •  Determine how core of massive star, during

DocID: 1uCW7 - View Document

Astronomy Assessment and TPS Questions: Star Formation and Lifetimes The total main sequence lifetime of stars like the Sun is about 1 million years.

DocID: 1uAWB - View Document

Magnetic Fields and Star Formation: Observations and Implications Richard Crutcher University of Illinois

DocID: 1uwzh - View Document