On the effective temperature of sunspot umbrae using beryllium hydride isotopomer lines

dc.contributor.author	Sangeetha, R
dc.contributor.author	Sriramachandran, P
dc.contributor.author	Bagare, S. P
dc.contributor.author	Rajamanickam, N
dc.contributor.author	Shanmugavel, R
dc.date.accessioned	2010-01-08T16:45:42Z
dc.date.available	2010-01-08T16:45:42Z
dc.date.issued	2009-12
dc.identifier.citation	Serbian Astronomical Journal, No. 179, pp. 95 - 99	en
dc.identifier.issn	1450-698X
dc.identifier.uri	http://hdl.handle.net/2248/4968
dc.description	Open Access
dc.description.abstract	A search for fourteen bands of the visible and infrared systems of the beryllium hydride isotopomers, in addition to the previously identified bands A - X(0, 0; 1, 1; 2, 2) for BeH, A - X(0, 0; 1, 1; 2, 2) for BeD and A - X(0, 0; 1, 1; 2, 2) for BeT molecules was conducted. The equivalent widths were measured for the well isolated identified lines of the strongest band and the effective temperatures were estimated for the systems for which the presence of hints is confirmed.	en
dc.language.iso	en	en
dc.publisher	Astronomical Observatory, Serbia	en
dc.relation.uri	http://saj.matf.bg.ac.yu/179.html	en
dc.rights	© Astronomical Observatory	en
dc.subject	Sunspots	en
dc.subject	Line: Identification	en
dc.title	On the effective temperature of sunspot umbrae using beryllium hydride isotopomer lines	en
dc.type	Article	en