Sign on

SAO/NASA ADS Astronomy Abstract Service

· Find Similar Abstracts (with default settings below)
· Electronic Refereed Journal Article (HTML)
· Full Refereed Journal Article (PDF/Postscript)
· arXiv e-print (arXiv:astro-ph/9812253)
· References in the article
· Citations to the Article (17) (Citation History)
· Refereed Citations to the Article
· SIMBAD Objects (223)
· NED Objects (224)
· Also-Read Articles (Reads History)
·
· Translate This Page
Title:
An Infrared Search for Extinguished Supernovae in Starburst Galaxies
Authors:
Grossan, Bruce; Spillar, Earl; Tripp, Robert; Pirzkal, Norbert; Sutin, Brian M.; Johnson, Paul; Barnaby, David
Publication:
The Astronomical Journal, Volume 118, Issue 2, pp. 705-718. (AJ Homepage)
Publication Date:
08/1999
Origin:
AJ
AJ Keywords:
ISM: DUST, EXTINCTION, GALAXIES: NUCLEI, GALAXIES: STARBURST, INFRARED RADIATION, INSTRUMENTATION: MISCELLANEOUS, STARS: SUPERNOVAE: GENERAL
DOI:
10.1086/300962
Bibliographic Code:
1999AJ....118..705G

Abstract

IR and radio-band observations of heavily extinguished regions in starburst galaxies suggest a high supernova (SN) rate associated with such regions. Optically measured SN rates may therefore underestimate the total SN rate by factors of up to 10, as a result of the very high extinction (A_B~10-20 mag) to core-collapse SNe in starburst regions. The IR/radio SN rates come from a variety of indirect means, however, which suffer from model dependence and other problems. We describe a direct measurement of the SN rate from a regular patrol of starburst galaxies done with K'-band imaging to minimize the effects of extinction. A collection of K'-band measurements of core-collapse SNe near maximum light is presented. Such measurements (excluding 1987A) are not well reported in the literature. Results of a preliminary K'-band search, using the MIRC camera at the Wyoming Infrared Observatory and an improved search strategy using the new ORCA optics, are described. A monthly patrol of a sample of IRAS bright (mostly starburst) galaxies within 25 Mpc should yield 1-6 SNe yr^-1, corresponding to the range of estimated SN rates. Our initial MIRC search with low resolution (2.2" pixels) failed to find extinguished SNe in the IRAS galaxies, limiting the SN rate outside the nucleus (at greater than 15" radius) to less than 3.8 far-IR SN rate units (SNe per century per 10^10 L_solar measured at 60 and 100 mum, or FIRSRU) at 90% confidence. The MIRC camera had insufficient resolution to search nuclear starburst regions, where starburst and SN activity is concentrated; therefore, we were unable to rigorously test the hypothesis of high SN rates in heavily obscured star-forming regions. We conclude that high-resolution nuclear SN searches in starburst galaxies with small fields are more productive than low-resolution, large-field searches, even for our sample of large (often several arcminutes) galaxies. With our ORCA high-resolution optics, we could limit the total SN rate to less than 1.3 FIRSRU at 90% confidence in 3 years of observations, lower than most estimates.
Bibtex entry for this abstract   Preferred format for this abstract (see Preferences)
   

Find Similar Abstracts:

Use: Authors
Title
Keywords (in text query field)
Abstract Text
Return: Query Results Return    items starting with number
Query Form
Database: Astronomy
Physics
arXiv e-prints