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Details for Revision 2
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Name
  V1104 Sco  
AAVSO UID
--  
Constellation
Scorpius Sequence
J2000.0
17 06 53.91 -42 36 39.7  (256.72463 -42.61103) Search nearby
B1950.0 17 03 20.54 -42 32 42.0
Galactic coord. 344.297 -1.157
Other names

(Internal only)
Please note that aliases shown in grey link to obsolete records.
AAVSO 1659-42 ASAS J170654-4236.6 CD-42 11834
CPD-42 7632 GSC 07877-00311 HD 326823
Hen 3-1330 PPM 762486  
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Variability type
SDOR:
Spectral type B1.5(e)
Mag. range
8.88 - 9.16 V
Discoverer --
Epoch
--
Outburst --
Period --
Rise/eclipse dur. --
Remarks
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1 Otero, Sebastian Alberto ASAS light curve (2001-2009) shows a bump in the descending branch reminiscent of CW stars. LTPV data (1988-1994) show the same light curve but with a shorter period of 6.119 d. This kind of periodic variability is not shown by the known SDOR stars. Double system with a CW component?
2 Otero, Sebastian Alberto Dormant SDOR star.
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References
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1 G.Pojmanski, Acta Astronomica 52, 397, 2002. 2002AcA....52..397P
2 S Doradus variables in the Galaxy and the Magellanic Clouds 2001A&A...366..508V
3 C.Sterken, O.Stahl, B.Wolf, Th.Szeifert, A.Jones, AsAp 303, No.3, 766,
1995.
1995A&A...303..766S
4 UBV photometry of OB+ stars in the southern Milky Way 1991ApJS...76.1033D
5 UBV photometry of OB+ stars in the southern Milky Way 1991ApJS...76.1033D
External Links
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Supporting Documents
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1 V1104 Sco light curve Otero, Sebastian Alberto 2010-01-02 01:09 UTC Light curve of the SDOR candidate showing its periodic behaviour. ASAS-3 data used.
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Revision History
Currently approved revision is checked. Click revision number to view details of that revision.
3 Otero, Sebastian Alberto 2010-01-02 01:09 UTC ASAS period for this star is essentially right. Range updated and epoch and period added from ASAS data.
2 Otero, Sebastian Alberto 2007-03-18 22:09 UTC New range from Drilling (1991) and LTPV data.
NOMAD position given.
1 Admin, VSX 2005-12-18 01:33 UTC Initial database population.