Spectral and UBV analysis of {epsilon} Aur Virtual Observatory Resource

Authors

1. Chadima P.
2. Harmanec P.
3. Bennett P.D.
4. Kloppenborg B.
5. Stencel R.
6. Yang S.,Bozic H.
7. Slechta M.
8. Kotkova L.
9. Wolf M.
10. Skoda P.
11. Votruba V.,Hopkins J.L.
12. Buil C.
13. Sudar D.

Published by

CDS

Abstract

A series of 353 red electronic spectra (from three observatories, mostly from 6300 to 6700{AA}) obtained between 1994 and 2010, and of 171 UBV photometric observations (from two observatories) of the 2010 eclipse, were analyzed in an effort to better understand epsilon Aur, the well-known, but still enigmatic eclipsing binary with the longest known orbital period (~27yrs).

Keywords

1. variable-stars
2. visible-astronomy
3. Wide-band photometry
4. spectroscopy

Bibliographic source Bibcode

2011A&A...530A.146C

See also HTML

https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/530/A146

IVOA Identifier IVOID

ivo://CDS.VizieR/J/A+A/530/A146

Document Object Identifer DOI

doi:10.26093/cds/vizier.35300146

Access

IVOA Table Access TAP

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