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Article: A multiwavelength study of the classical nova V4169 Sagittarii

TitleA multiwavelength study of the classical nova V4169 Sagittarii
Authors
KeywordsSTARS: ABUNDANCES
CIRCUMSTELLAR MATTER
STARS: INDIVIDUAL: V4169 SGR
NOVAE
CATACLYSMIC VARIABLES -IR: STARS
UV: STARS
Issue Date1995
Citation
Astronomy and Astrophysics, 1995, v. 296, p. 439-439 How to Cite?
AbstractWe present multiwavelength observations of V4169 Sgr (Nova Sgr 92#2) from 1000A to 2cm for the first year following visual maximum. V4169 Sgr was an `Fe II' type nova, and evolved from P^0^_fe_ to N_0_ in the Tololo nova classification scheme. The ultraviolet spectrum was very similar to that of nova PW Vul, and the near infra-red spectrum was dominated by Lybeta pumped Oi emission in the early decline. There was significant apparent deceleration of absorption lines before optical maximum. High resolution optical spectroscopy reveal unusual details of the evolution of blue-shifted P Cygni absorptions; we show that these are consistent with the advance of an ionisation front through the absorbing material. The evolution of absorption systems and emission line profiles are consistent with accelerating wind models of nova ejection. We find an extinction of E(B-V)=0.35+/-0.05, and a distance of ~6.5kpc. The nova shows significant enrichment of helium and nitrogen relative to solar, but not of carbon or oxygen; however our abundances are probably underestimated.
Persistent Identifierhttp://hdl.handle.net/10722/211199
ISSN
2014 Impact Factor: 4.378
2015 SCImago Journal Rankings: 2.446

 

DC FieldValueLanguage
dc.contributor.authorScott, AD-
dc.contributor.authorDuerbeck, HW-
dc.contributor.authorEvans, A-
dc.contributor.authorChen, AL-
dc.contributor.authorde Martino, D-
dc.contributor.authorHjellming, R-
dc.contributor.authorKrautter, J-
dc.contributor.authorLaney, D-
dc.contributor.authorParker, QA-
dc.contributor.authorRawlings, JMC-
dc.contributor.authorVan Winckel, H-
dc.date.accessioned2015-07-08T03:22:57Z-
dc.date.available2015-07-08T03:22:57Z-
dc.date.issued1995-
dc.identifier.citationAstronomy and Astrophysics, 1995, v. 296, p. 439-439-
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/10722/211199-
dc.description.abstractWe present multiwavelength observations of V4169 Sgr (Nova Sgr 92#2) from 1000A to 2cm for the first year following visual maximum. V4169 Sgr was an `Fe II' type nova, and evolved from P^0^_fe_ to N_0_ in the Tololo nova classification scheme. The ultraviolet spectrum was very similar to that of nova PW Vul, and the near infra-red spectrum was dominated by Lybeta pumped Oi emission in the early decline. There was significant apparent deceleration of absorption lines before optical maximum. High resolution optical spectroscopy reveal unusual details of the evolution of blue-shifted P Cygni absorptions; we show that these are consistent with the advance of an ionisation front through the absorbing material. The evolution of absorption systems and emission line profiles are consistent with accelerating wind models of nova ejection. We find an extinction of E(B-V)=0.35+/-0.05, and a distance of ~6.5kpc. The nova shows significant enrichment of helium and nitrogen relative to solar, but not of carbon or oxygen; however our abundances are probably underestimated.-
dc.languageeng-
dc.relation.ispartofAstronomy and Astrophysics-
dc.subjectSTARS: ABUNDANCES-
dc.subjectCIRCUMSTELLAR MATTER-
dc.subjectSTARS: INDIVIDUAL: V4169 SGR-
dc.subjectNOVAE-
dc.subjectCATACLYSMIC VARIABLES -IR: STARS-
dc.subjectUV: STARS-
dc.titleA multiwavelength study of the classical nova V4169 Sagittarii-
dc.typeArticle-
dc.identifier.emailParker, QA: quentinp@hku.hk-
dc.identifier.authorityParker, QA=rp02017-
dc.identifier.volume296-
dc.identifier.spage439-
dc.identifier.epage439-

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