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  FS CMa  
000-BCV-035 (1747 observations)  
Canis Major Sequence
06 28 17.42 -13 03 11.1  (97.07258 -13.05308) Search nearby
B1950.0 06 25 59.06 -13 01 12.7
Galactic coord. 222.088 -10.976
Other names

(Internal only)
AAVSO 0623-12 ASAS J062817-1303.2 BD-12 1500
HD 45677 HIP 30800 IRAS 06259-1301
MWC 142 RAFGL 5195 SAO 151534
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Variability type
Spectral type B2IVep
Mag. range
7.55 - 8.58 V
Discoverer --
Outburst --
Period --
Rise/eclipse dur. --
Some references may be clicked to view in new window. Roll over index number to view submission details.
1 GCVS Team Extended shell of gas and dust. Emissions of [FeII], [NiII], [CrII], [SII], [OI], FeII. IR excess (1.6 - 20 mkm). P Cyg profiles of Balmer lines vary in the time scale of hours. Brightness varies from night to night by 0.1m and during a night by 0.03m, sometimes in correlation with spectral changes [J.P.Swings, R.Barbier, M.Klutz, A.Surdej, J.Surdej, AsAp 90, 116, 1980.]. Spectral studies [J.P.Swings, AsAp 26, N3, 443, 1973., A.R.Hyland, Proc ASA 2, N1, 14, 1971., F.Ciatti, S.D'Odorico, A.Mammano, AsAp 34, 181, 1974.].
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1 Miroshnichenko, A. S., 2007, Toward Understanding the B[e] Phenomenon. I.
Definition of the Galactic FS CMa Stars
2 C. Koen, L. Eyer, 2002, MNRAS 331, 45 2002MNRAS.331...45K
3 The All Sky Automated Survey 2002AcA....52..397P
4 J.P.Swings, D.A.Allen, ApJ 167, L41, 1971. 1971ApJ...167L..41S
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Revision History
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6 Otero, Sebastian Alberto 2014-02-15 23:54 UTC Spurious period from 2002MNRAS.331...45K deleted.
5 Admin, VSX 2013-05-03 19:16 UTC Update from [2002MNRAS.331...45K].
4 Otero, Sebastian Alberto 2013-03-26 16:11 UTC Type from 2007ApJ...667..497M.
3 Otero, Sebastian Alberto 2011-11-12 04:38 UTC Maximum magnitude from ASAS-3 data.
2 Admin, VSX 2010-01-04 23:43 UTC Position updated from the GCVS version of November 2009.
1 Admin, VSX 2005-12-17 20:33 UTC Initial upload.