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

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