Spectroscopic monitoring of the symbiotic star BX monocerotis

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5777

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DC Field	Value	Language
dc.contributor.author	Anupama, G. C	-
dc.contributor.author	Kamath, U. S	-
dc.contributor.author	Gurugubelli, U. K	-
dc.contributor.author	Mikołajewska, J	-
dc.date.accessioned	2012-06-08T16:42:00Z	-
dc.date.available	2012-06-08T16:42:00Z	-
dc.date.issued	2012	-
dc.identifier.citation	Baltic Astronomy, Vol. 21, No. 1-2, pp. 172-179	en
dc.identifier.issn	1392-0049	-
dc.identifier.uri	http://hdl.handle.net/2248/5777	-
dc.description	Restricted Access	en
dc.description.abstract	Low resolution optical spectra of the symbiotic star BX Monocerotis in the 3500--9000 A range obtained during 1999--2010 are described. The spectrum of BX Mon at all phases is dominated by the cool component, with a red continuum and TiO absorption. Emission lines, predominantly due to H I, He I, He II, Fe II, Ca II and [O III] are seen superimposed on the spectrum of the M5 III star, with variable intensities. The observed variations in the spectra seem to be correlated with the orbital phases.	en
dc.language.iso	en	en
dc.publisher	Vilnius University and the Lithuanian Astronomical Union	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2012BaltA..21..172A	en
dc.rights	© Vilniaus Universitetas ir Lietuvos astronomu sajunga, 2012	en
dc.subject	Stars: binaries: symbiotic	en
dc.subject	Stars: individual (BX Mon)	en
dc.title	Spectroscopic monitoring of the symbiotic star BX monocerotis	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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