Outbursts in the Be star HR 2501 Virtual Observatory Resource

Authors

1. Carrier F.
2. Burki G.

Published by

CDS

Abstract

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.

Keywords

1. variable-stars
2. radial-velocity
3. visible-astronomy
4. narrow-band-photometry

Bibliographic source Bibcode

2003A&A...401..271C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/401/271

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/401/271

Document Object Identifer DOI

doi:10.26093/cds/vizier.34010271

Access

Web browser access HTML

http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/401/271
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/401/271
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/401/271

IVOA Table Access TAP

http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).