X-ray flares on the UV Ceti-type star CC Eridani: a “peculiar” time-evolution of spectral parameters-Reference-Cited by-同舟云学术

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X-ray flares on the UV Ceti-type star CC Eridani: a “peculiar” time-evolution of spectral parameters

Published:2007-06-18 Issue:3 Volume:471 Page:929-939
ISSN:0004-6361
Container-title:Astronomy & Astrophysics
language:
Short-container-title:A&A

Author:

Crespo-Chacón I.,Micela G.,Reale F.,Caramazza M.,López-Santiago J.,Pillitteri I.

Publisher

EDP Sciences

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://www.aanda.org/10.1051/0004-6361:20077601/pdf

Reference99 articles.

1. Abundances of the elements: Meteoritic and solar

2. Arnaud, K. 2004, AAS/High Energy Astrophysics Division, 8, #16.29

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1. Swift and XMM–Newton observations of an RS CVn-type eclipsing binary SZ Psc: superflare and coronal properties;Monthly Notices of the Royal Astronomical Society;2022-09-30

2. Stellar activity with LAMOST. III. Temporal variability pattern in Pleiades, Praesepe, and Hyades;Monthly Notices of the Royal Astronomical Society;2020-05-21

3. X-Ray Superflares on CC Eri;The Astrophysical Journal;2017-05-12

4. A survey of stellar X-ray flares from theXMM-Newtonserendipitous source catalogue: HIPPARCOS-Tycho cool stars;Astronomy & Astrophysics;2015-08-27

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