Near-infrared spectroscopy of nova Sagittarii 1998

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