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  5. On the Frequency of Occurrence of Recurrent Novae and Their Role as Type IA Supernova Progenitors
 

On the Frequency of Occurrence of Recurrent Novae and Their Role as Type IA Supernova Progenitors

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
1996
Author(s)
DELLA VALLE, Massimo  
•
Livio, Mario
DOI
10.1086/178139
Abstract
We have determined the frequency of occurrence of recurrent novae (RNe) for the Galaxy, M31, and the LMC. We find that the ratio between the rate of outbursts of recurrent and classical novae (CNe) is in the range n_out_(RNe)/n_out_(CNe) ~ 0.1-0.3. The implications of this result for the realization frequency of RNe as potential progenitors of Type Ia supernovae are also discussed. RNe are not the major class of progenitors of Type Ia supernovae.
Volume
473
Issue
1 PART I
Start page
240
Uri
http://hdl.handle.net/20.500.12386/32689
Url
https://iopscience.iop.org/article/10.1086/178139
https://api.elsevier.com/content/abstract/scopus_id/21444455940
Issn Identifier
0004-637X
Ads BibCode
1996ApJ...473..240D
Rights
open.access
File(s)
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document.pdf

Description
Pdf editoriale
Size

59.81 KB

Format

Adobe PDF

Checksum (MD5)

b0c811708890c07edb08adf40725bc0b

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