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 |