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Article: The recurrent nova V394 Coronae Austrinae - The 1987 outburst

TitleThe recurrent nova V394 Coronae Austrinae - The 1987 outburst
Authors
Sekiguchi, KCatchpole, RMFairall, APFeast, MWKilkenny, DLaney, CDLloyd Evans, TMarang, FParker, QA
KeywordsEmission Spectra
Novae
Stellar Spectra
Astronomical Photometry
Astronomical Spectroscopy
H Alpha Line
Light Curve
Issue Date1989
PublisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/
Citation
Monthly Notices of the Royal Astronomical Society, 1989, v. 236, p. 611-619 How to Cite?
DOI: http://dx.doi.org/10.1093/mnras/236.3.611
AbstractOptical and infrared observations of the 1987 outburst of the recurrent nova V394 Coronae Austrinae are reported. The amplitude of the outburst (Delta V of about 11 mag) is comparable to that of classical novae. The fast optical decline rate and the gross spectral characteristics of V394 CrA closely resemble those of U Sco. Compared to U Sco, the broad emission bands in the early decline are slightly narrower, and the late optical decline and spectral development are slower. Implications for thermonuclear runaway models are mentioned.
Persistent Identifierhttp://hdl.handle.net/10722/211173
ISSN
0035-8711
2021 Impact Factor: 5.235
2020 SCImago Journal Rankings: 2.058
ISI Accession Number ID
WOS:A1989T036400007

 

DC FieldValueLanguage
dc.contributor.authorSekiguchi, K-
dc.contributor.authorCatchpole, RM-
dc.contributor.authorFairall, AP-
dc.contributor.authorFeast, MW-
dc.contributor.authorKilkenny, D-
dc.contributor.authorLaney, CD-
dc.contributor.authorLloyd Evans, T-
dc.contributor.authorMarang, F-
dc.contributor.authorParker, QA-
dc.date.accessioned2015-07-08T03:22:34Z-
dc.date.available2015-07-08T03:22:34Z-
dc.date.issued1989-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 1989, v. 236, p. 611-619-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/10722/211173-
dc.description.abstractOptical and infrared observations of the 1987 outburst of the recurrent nova V394 Coronae Austrinae are reported. The amplitude of the outburst (Delta V of about 11 mag) is comparable to that of classical novae. The fast optical decline rate and the gross spectral characteristics of V394 CrA closely resemble those of U Sco. Compared to U Sco, the broad emission bands in the early decline are slightly narrower, and the late optical decline and spectral development are slower. Implications for thermonuclear runaway models are mentioned.-
dc.languageeng-
dc.publisherOxford University press. The Journal's web site is located at http://www.oxfordjournals.org/our_journals/mnras/-
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society-
dc.subjectEmission Spectra-
dc.subjectNovae-
dc.subjectStellar Spectra-
dc.subjectAstronomical Photometry-
dc.subjectAstronomical Spectroscopy-
dc.subjectH Alpha Line-
dc.subjectLight Curve-
dc.titleThe recurrent nova V394 Coronae Austrinae - The 1987 outburst-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.description.naturelink_to_OA_fulltext-
dc.identifier.doi10.1093/mnras/236.3.611-
dc.identifier.scopuseid_2-s2.0-0000726326-
dc.identifier.volume236-
dc.identifier.spage611-
dc.identifier.epage619-
dc.identifier.isiWOS:A1989T036400007-
dc.identifier.issnl0035-8711-

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