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[vsnet-be 17] V862 Outburst Refs
The original Bakos V862 Sco = HD 160202 ref. appears to be in the
following book:
1967 BAKOS NON PERIODIC PHENOMENA VARIABLE STARS ED DETRE REIDEL 1967
unfortunately no page number is given.
Another reference [besides the S&T one from an earlier post by Taichi
Kato] for comments on this star by G A Bakos is:
Commumications of the Konkoly Observatory, No. 65 (Vol. VI, 1), p.
159-160 (1969)
Meanwhile, an abstract search using Bakos as author gives this for HD
160202 in 1985 [but unfortunately no archived article]:
[Abstarct from NASA ADS service at adsabs.harvard.edu]
==============================================snip
> Title: Light variations of the B-type star HD 160202
> Authors: Bakos, G. A.
> Affiliation: Waterloo Univ. (Ontario).
> Journal: In NASA. Goddard Space Flight Center The Origin of Nonradiative
> Heating/Momentum in Hot Stars p 62-65 (SEE N85-17755 08-88)
> Publication Date: 01/1985
> Category: Astronomy
> Origin: STI
> NASA/STI Keywords: B STARS, STELLAR FLARES, STELLAR LUMINOSITY, GALACTIC
> CLUSTERS, PHOTOMETRY, STELLAR ENVELOPES, VARIATIONS
> Bibliographic Code: 1985onhm.rept...62B
>
> Abstract
>
> Light variations of the B-type star HD 160202 in the galactic cluster M6 are presented. A flare type
> increase in brightness by about three magnitudes in a time interval of 40 minutes was recorded. It is
> shown that a B-type star in the galactic cluster M 6 went through the process of shell formation and a
> flare type increase in brightness in a time interval of three years. Similar cases associated with B-type
> stars were reported in the past; however, they represent sporadic and accidental observations. The
> observations presented here show a flare-type event with a resolution of five minutes.
===========================================================endsnip
The note of rapid flaring further biases me towards a compact companion,
though Bakos evidently sees it as some kind of flare star.
John
vsnet-adm@kusastro.kyoto-u.ac.jp
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