Solar Photospheric Models and the Rotational Temperatures of THE C/sub2/ and MgH Molecules

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/533

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DC Field	Value	Language
dc.contributor.author	Sinha, K	-
dc.contributor.author	Shukla, D. S	-
dc.contributor.author	Tripathi, B. M	-
dc.date.accessioned	2005-08-13T06:32:25Z	-
dc.date.available	2005-08-13T06:32:25Z	-
dc.date.issued	1979-06	-
dc.identifier.citation	BASI, Vol. 7, No. 2, pp. 38-42	en
dc.identifier.uri	http://hdl.handle.net/2248/533	-
dc.description.abstract	Four photospheric models have been utilized to derive model based rotational temperatures of the (0-0) band of the Swan system of C/sub2/ and that of the green system of the MgH molecules. The dissociation energies were varied within reasonable limits to assess their influence on the derived temperatures. It is found that observations are not consistent with the model based results. The need for more refined photospheric models is emphasized.	en
dc.format.extent	792536 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	-
dc.publisher	Astronomical Society of India	en
dc.subject	Solar Photospheric Models	en
dc.subject	Rotational Temperature	en
dc.title	Solar Photospheric Models and the Rotational Temperatures of THE C/sub2/ and MgH Molecules	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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