Pulsation stability of helium-rich subdwarf B stars

Details Pulsation stability of helium-rich subdwarf B stars Pulsation stability of helium-rich subdwarf B stars

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.291..435a&link_type=abstract

Astrophysics and Space Science, v. 291, Issue 3, p. 435-439 (2004).

Astronomy and Astrophysics

Astrophysics

2

Helium-Rich Subdwarf B Stars, Pulsations, Photometry

Scientific paper

We present results of the pulsation monitoring of helium-rich subdwarf B
(He-sdB) stars using high-speed differential photometry observations
made with the SAAO (1.0m), NOT (2.6m) and the IAC80 (0.8m) telescopes.
Although we did not find a pulsator in our sample of He-sdB stars, some
of the stars show hints of pulsations which need further investigation.

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