Published October 2, 2003
| public
Book Section - Chapter
Core-Collapse Supernova Progenitors in Hubble Space Telescope Images
Abstract
Determining which stars give rise to supernovae (SNe) is key to SN research and stellar evolution studies. Without knowledge of SN progenitors, many of the conclusions and inferences made about the connection between SNe and important problems in astrophysics stand on precarious ground. The main obstacle is that a SN leaves few traces of the star that exploded.
Additional Information
© 2003 Springer-Verlag Berlin Heidelberg. First Online: 02 October 2003. This publication makes use of data products from 2MASS, a joint project of the University of Massachusetts and IPAC/Caltech, funded by NASA and NSF; of the NASA/IPAC Extragalactic Database (NED), operated by JPL/Caltech for NASA; and of LEDA (http://leda.univ-lyon.fr). A.V.F.'s group at UC Berkeley is supported by NSF grant AST-9987438, the Sylvia and Jim Katzman Foundation, and NASA/HST grants AR-8754, AR-9529, and GO-8602.Additional details
- Eprint ID
- 103826
- DOI
- 10.1007/10828549_6
- Resolver ID
- CaltechAUTHORS:20200610-125339255
- NASA/JPL/Caltech
- AST-9987438
- NSF
- Sylvia and Jim Katzman Foundation
- AR-8754
- NASA
- AR-9529
- NASA
- GO-8602
- NASA
- Created
-
2020-06-10Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)
- Series Name
- ESO Astrophysics Symposia