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The EC14026 Stars - Pulsating Hot Subdwarfs

Published online by Cambridge University Press:  08 February 2017

C. Koen ,
D. O'Donoghue ,
D. Kilkenny  and
R.S. Stobie
C. Koen
Affiliation:
South African Astronomical Observatory, PO Box 9, Observatory, 7935, Cape, South Africa
D. O'Donoghue
Affiliation:
South African Astronomical Observatory, PO Box 9, Observatory, 7935, Cape, South Africa
D. Kilkenny
Affiliation:
South African Astronomical Observatory, PO Box 9, Observatory, 7935, Cape, South Africa
R.S. Stobie
Affiliation:
South African Astronomical Observatory, PO Box 9, Observatory, 7935, Cape, South Africa

Extract

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The Edinburgh-Cape Blue Object Survey (Stobie et al. 1997a) is a southern hemisphere survey to discover hot, blue stellar objects brighter than B=18 at galactic latitudes more than 30° from the galactic plane. The main categories of object detected are hot subdwarfs, white dwarfs, blue horizontal branch stars, apparently normal B stars, cataclysmic variables and (stellar-like) active galactic nuclei. Over 50% of the EC Survey comprises hot subdwarfs.

Type
VI. Asteroseismology II
Information
Symposium - International Astronomical Union , Volume 185: New Eyes to See Inside the Sun and Stars , 1998 , pp. 361 - 366
Copyright
Copyright © Kluwer 1998 

References

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