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Astron. Astrophys. 349, 537-545 (1999)
Light variations of massive stars ( Cygni variables) *
XVII. The LMC supergiants R 74 (LBV), R 78, HD 34664 = S 22
(B[e]/LBV), R 84 and R 116 (LBV?)
A.M. van Genderen 1 and
C. Sterken ** 2
1 Leiden Observatory, Postbus 9513, 2300RA Leiden, The Netherlands (genderen@strw.leidenuniv.nl)
2 University of Brussels (VUB), Pleinlaan 2, B-1050 Brussels, Belgium
Received 21 April 1999 / Accepted 3 June 1999
Abstract
Multi-colour photometry (Walraven system) of five super- and
hypergiants in the LMC, viz. R 74, R 78, HD 34664, R 84 and R 116, is
searched for variability and periods, and discussed. Apart from R 84,
of which the claimed variability in the past must be due to a number
of faint field stars at the edge of the apertures, all are
variable.
R 74 and HD 34664 are weak-active LBVs with superimposed
microvariations. HD 34664 is the second known B[e] star which is also
an LBV. The first reported one is R 4 in the SMC. This could alter
some views on the evolutionary history of B[e] stars and LBVs.
R 78 is an Cyg variable, but
presumably no LBV. R 116 appears to be a close counterpart of the
galactic ex-/dormant LBV Sco,
also showing an intricate
Cyg-type multi-period
microvariability.
Key words: stars: individual: R 116 = HDE 269700; R 74
= HDE 268939; R 78 = HDE 269050; R 84 = HDE 269227;
S 22 = HD 34664
galaxies: Magellanic Clouds
* Based on observations obtained at the European Southern Observatory at La Silla, Chile
** Belgian Fund for Scientific Research (FWO)
Send offprint requests to: A.M. van Genderen
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© European Southern Observatory (ESO) 1999
Online publication: September 2, 1999
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