Outbursts in the Be star HR 2501 (Carrier+, 2003)

Details Outbursts in the Be star HR 2501 (Carrier+, 2003) Outbursts in the Be star HR 2501 (Carrier+, 2003)

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..34010271c&link_type=abstract

VizieR On-line Data Catalog: J/A+A/401/271. Originally published in: 2003A&A...401..271C

Physics

Stars: Variable, Radial Velocities, Photometry: Geneva

Scientific paper

Several mostly unrelated periods or time scales characterize the variability of HR 2501. This star is a new lambda Eri star with a period of 0.79187d. This star also exhibits a mid- to long-term variability of characteristic time ~500d, most probably a consequence of the recurrent outbursts of matter from the rapidly rotating Be star towards its disk.
(2 data files).

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