V2493 Cyg BVRI long term photometry

DOI

We present new results from optical photometric and spectroscopic observations of the eruptive pre-main sequence star V2493 Cyg (HBC 722). The object has continued to undergo significant brightness variations over the past few months and is an ideal target for follow-up observations.

Identifier
DOI http://doi.org/10.26093/cds/vizier.35420043
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/542/A43
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/542/A43
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/542/A43
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/542/A43
Provenance
Creator Semkov E.H.; Peneva S.P.; Munari U.; Tsvetkov M.K.; Jurdana-Sepic R.,de Miguel E.; Schwartz R.D.; Dimitrov D.P.; Kjurkchieva D.P.; Radeva V.S.
Publisher CDS
Publication Year 2012
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics; Stellar Astronomy