Long-term BVRI photometry of V1704 Cygni Virtual Observatory Resource

Authors
  1. Ibryamov S.
  2. Semkov E.
  3. Peneva S.
  4. Karadeniz U.
  5. Published by
    CDS
Abstract

Results from BVRI photometric observations of the pre-main sequence star V1704 Cyg collected during the time period from August 2010 to December 2017 are presented. The star is located in the star-forming HII region IC 5070 and it exhibits photometric variability in all optical passbands. After analysing the obtained data, V1704 Cyg is classified as a classical T Tauri star.

Keywords
  1. variable-stars
  2. pre-main-sequence-stars
  3. infrared-photometry
  4. visible-astronomy
  5. Wide-band photometry
Bibliographic source Bibcode
2018BAJ....29...10I
See also HTML
https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/BAJ/29.10
IVOA Identifier IVOID
ivo://CDS.VizieR/J/other/BAJ/29.10

Access

Web browser access HTML
http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/other/BAJ/29.10
https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/BAJ/29.10
http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/BAJ/29.10
IVOA Table Access TAP
http://tapvizier.cds.unistra.fr/TAPVizieR/tap
Run SQL-like queries with TAP-enabled clients (e.g., TOPCAT).

History

2019-01-03T09:08:22Z
Resource record created
2019-01-03T09:08:22Z
Created
2020-01-31T15:23:27Z
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