Photometry of FG Sge at the ejection state Virtual Observatory Resource

Authors
  1. Arkhipova V.P.
  2. Esipov V.F.
  3. Ikonnikova N.P.
  4. Komissarova G.V.,Shugarov S.Yu.
  5. Published by
    CDS
Abstract

New photometric observations of the variable star FG Sge, a rapidly evolving planetary nebula nucleus, were performed in 2003-2008. On 230 nights, we obtained 86 UBV and 155 BVRI (or Rc, Ic) magnitude estimates. The maximum amplitude of the V-band light variations was >8mag. Six deep minima and four high maxima were observed.

Keywords
  1. supergiant-stars
  2. visible-astronomy
  3. Wide-band photometry
  4. spectroscopy
Bibliographic source Bibcode
2009PAZh...35..592A
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/35/592
IVOA Identifier IVOID
ivo://CDS.VizieR/J/PAZh/35/592

Access

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

History

2010-02-06T08:20:03Z
Resource record created
2010-02-06T08:20:03Z
Created
2017-06-27T06:38:49Z
Updated

Contact

Name
CDS support team
Postal Address
CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France
E-Mail
cds-question@unistra.fr