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Spectroscopic studies of R CrB during light minima - Absorption spectrum

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dc.contributor.author Kameswara Rao, N
dc.contributor.author Giridhar, S
dc.contributor.author Ashoka, B. N
dc.date.accessioned 2008-09-17T12:16:38Z
dc.date.available 2008-09-17T12:16:38Z
dc.date.issued 1990-05
dc.identifier.citation Monthly Notices Royal Astronomical Society, Vol. 244, No.1, pp. 29 - 34 en
dc.identifier.issn 0035-8711
dc.identifier.uri http://hdl.handle.net/2248/3717
dc.description.abstract R CrB was observed during the 1986 shallow minimum to study the spectral changes taking place during light minimum as compared with the spectrum at maximum light. The absorption spectrum at this minimum is very similar to the spectrum seen during the early decline of the 1963 light minimum. An enhancement of molecular bands of C2, CN, and low excitation atomic lines is found during these phases. An absorption feature at 4050.5A is also noted, probably due to C3 in the early decline of the 1963 and 1986 minima. Calculations do not indicate any drastic change in effective temperature and microturbulence between light maximum and minimum. It appears that regions with enhanced molecular absorptions are required to explain the absorption spectrum during light minimum. en
dc.language.iso en en
dc.publisher Royal Astronomical Society en
dc.relation.uri http://ads.iucaa.ernet.in/abs/1990MNRAS.244...29K en
dc.subject Absorption spectra en
dc.subject Astronomical spectroscopy en
dc.subject R coronae borealis stars en
dc.subject Stellar evolution en
dc.subject Carbon en
dc.subject IUE en
dc.subject Light curve en
dc.subject Spectral line width en
dc.subject Stellar spectra en
dc.title Spectroscopic studies of R CrB during light minima - Absorption spectrum en
dc.type Article en


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