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http://hdl.handle.net/2248/2759
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DC Field | Value | Language |
---|---|---|
dc.contributor.author | Kameswara Rao, N | - |
dc.contributor.author | Lambert, D. L | - |
dc.date.accessioned | 2008-07-21T09:26:09Z | - |
dc.date.available | 2008-07-21T09:26:09Z | - |
dc.date.issued | 1993-05 | - |
dc.identifier.citation | Astronomical Journal, Vol. 105, No. 5, pp. 1915 - 1926 | en |
dc.identifier.issn | 0004-6256 | - |
dc.identifier.uri | http://hdl.handle.net/2248/2759 | - |
dc.description.abstract | The R Coronae Borealis star V854 Cen was observed at minimum light (V about 15) at high spectral resolution from 5480 to 7070 A. The spectrum consists of three components: a continuum devoid of photospheric lines, a collection of sharp emission lines of Sc II, Ti II, Y II, and Ba II, and broad emission lines of forbidden O I, forbidden N II, forbidden S II, H-alpha, Na D, and C2 Swan bands. A low resolution spectrum reveals additional lines of Ca II, forbidden C I, and other species. The sharp emission lines are considered to be chromospheric lines. The broad lines with a full width of 400-500 km/s come from an extended region with a temperature of about 7000 K, but an electron density of 50/cu cm or less. It is suggested that V854 Cen may be a bipolar nebula. | en |
dc.format.extent | 2008015 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | American Astronomical Society | en |
dc.relation.uri | http://adsabs.harvard.edu/abs/1993AJ....105.1915K | en |
dc.subject | Absorption spectra | en |
dc.subject | Astronomical spectroscopy | en |
dc.subject | Emission spectra | en |
dc.subject | R coronae borealis stars | en |
dc.subject | Charge coupled devices | en |
dc.subject | Chromosphere | en |
dc.subject | High resolution | en |
dc.subject | Nebulae | en |
dc.subject | Photosphere | en |
dc.subject | Spectral line width | en |
dc.subject | Spectral resolution | en |
dc.title | High resolution spectroscopy of the R Coronae Borealis star, V854 Centauri, during a deep minimum | en |
dc.type | Article | en |
Appears in Collections: | IIAP Publications |
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