Tidally trapped pulsations in a close binary star system discovered by TESS-Reference-Cited by-同舟云学术

Tidally trapped pulsations in a close binary star system discovered by TESS

Published:2020-03-09 Issue:7 Volume:4 Page:684-689
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Handler G.^ORCID,Kurtz D. W.,Rappaport S. A.,Saio H.,Fuller J.,Jones D.^ORCID,Guo Z.^ORCID,Chowdhury S.,Sowicka P.^ORCID,Aliçavuş F. Kahraman,Streamer M.,Murphy S. J.^ORCID,Gagliano R.^ORCID,Jacobs T. L.^ORCID,Vanderburg A.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-020-1035-1.pdf

Reference35 articles.

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2. Aerts, C., Christensen-Dalsgaard, J. & Kurtz, D. W. Asteroseismology (Springer, 2010).

3. Cowling, T. G. The non-radial oscillations of polytropic stars. Mon. Not. R. Astron. Soc. 101, 367–375 (1941).

4. Handler, G. et al. Discovery and analysis of p-mode and g-mode oscillations in the A-type primary of the eccentric binary HD 209295. Mon. Not. R. Astron. Soc. 333, 262–279 (2002).

5. Welsh, W. F. et al. KOI-54: the Kepler discovery of tidally excited pulsations and brightenings in a highly eccentric binary. Astrophys. J. 197, 4 (2011).

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