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Near-infrared spectroscopy of nova Sagittarii 1998

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dc.contributor.author Ashok, N. M
dc.contributor.author Chandrasekhar, T
dc.date.accessioned 2008-02-29T09:31:22Z
dc.date.available 2008-02-29T09:31:22Z
dc.date.issued 2000
dc.identifier.citation BASI, Vol. 28, No. 2, pp. 265 - 267 en
dc.identifier.uri http://hdl.handle.net/2248/2098
dc.description.abstract Near-infrared spectra of Fe-II type nova, Nova Sagittarii 1998 obtained during the period 30 to 70 days after the discovery date are presented. The near infrared spectrum is dominated by emission lines of hydrogen and accompanied by lines of CI, OI and NI. The 1.129 ?m OI line excited by Lyman fluroscence is prominently seen in our first spectrum obtained in April 1998. In addition the OI line at 1.316 ?m is also detected indicating the presence of UV continuum fluroscence. en
dc.format.extent 169335 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.relation.uri http://adsabs.harvard.edu/abs/2000BASI...28..265A en
dc.subject Spectroscopy en
dc.subject Fe-II type nova en
dc.title Near-infrared spectroscopy of nova Sagittarii 1998 en
dc.type Article en

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