Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7090
Full metadata record
DC FieldValueLanguage
dc.contributor.authorRaj, A-
dc.contributor.authorDas, R. K-
dc.contributor.authorWalter, F. M.-
dc.date.accessioned2017-03-15T06:58:53Z-
dc.date.available2017-03-15T06:58:53Z-
dc.date.issued2017-02-01-
dc.identifier.citationThe Astrophysical Journal, Vol. 835, No. 2, 274en_US
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/7090-
dc.descriptionRestricted Accessen_US
dc.description.abstractWe present optical spectrophotometric and near-infrared (NIR) photometric observations of the nova V2676 Oph covering the period from 2012 March 29 through 2015 May 8. The optical spectra and photometry of the nova have been taken from SMARTS and Asiago; the NIR photometry was obtained from SMARTS and Mt. Abu. The spectra were dominated by strong H i lines from the Balmer series, Fe ii, N i, and [O i] lines in the initial days, typical of an Fe ii type nova. The measured FWHM for the Hβ and Hα lines was 800–1200 km s−1. There was pronounced dust formation starting 90 days after the outburst. The J − K color was the largest among recent dust-forming novae.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.relation.urihttps://doi.org/10.3847/1538-4357/835/2/274-
dc.rights© The American Astronomical Society-
dc.subjectInfrared: starsen_US
dc.subjectLine: identificationen_US
dc.subjectNovae, cataclysmic variablesen_US
dc.subjectStars: individual ( V2676 Oph )en_US
dc.subjectTechniques: spectroscopicen_US
dc.titleOptical and Near-infrared Study of Nova V2676 Oph 2012en_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

Files in This Item:
File Description SizeFormat 
Optical and Near-infrared Study of Nova V2676 Oph 2012.pdfRestricted Access438.17 kBAdobe PDFView/Open    Request a copy


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.