Can HeH(+) molecule be present in solar photosphere

dc.contributor.author	Gaur, V. P
dc.contributor.author	Joshi, G. C
dc.contributor.author	Pande, M. C
dc.date.accessioned	2007-03-21T06:52:58Z
dc.date.available	2007-03-21T06:52:58Z
dc.date.issued	1992
dc.identifier.citation	BASI, Vol. 20, pp. 61-63	en
dc.identifier.uri	http://hdl.handle.net/2248/1459
dc.description.abstract	The equivalent widths of the P and R branch lines of the fundamental vibration-rotation band arising from the ground state of HeH(+) have been calculated in a chosen photospheric model. The resulting equivalent widths suggest that the solar spectrum in the infrared region should be searched for, resolving the question regarding the presence or absence of HeH(+) in the sun	en
dc.format.extent	248015 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	Solar spectra	en
dc.title	Can HeH(+) molecule be present in solar photosphere	en
dc.type	Article	en