On the detectibility of HeH⁺ in the solar photospheric spectrum

dc.contributor.author	Sinha, K.
dc.date.accessioned	2010-01-08T05:39:14Z
dc.date.available	2010-01-08T05:39:14Z
dc.date.issued	1994
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/410
dc.description.abstract	In a recent publication of the Bulletin of the Astronomical Society of India, the possibility of detection of the (1-0) vibration-rotation lines of HeH⁺ molecules in the solar photospheric spectrum has been suggested. Taking cue, the Photometric Atlas of the Solar Spectrum from 1850 to 10,000 cm⁻¹ was scanned for the suggested lines in the present preliminary investigation. It is tentatively concluded that (i) it seems rather difficult to detect the HeH⁺ lines and (ii) observations from above the terrestrial atmosphere may be required for firm conclusion.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	basi22-143
dc.subject	Photospheric spectrum, Photospheric atlas, Ionic molecules	en_US
dc.title	On the detectibility of HeH⁺ in the solar photospheric spectrum	en_US
dc.type	Article	en_US