Four New Variable Stars in Ophiuchus

Details Four New Variable Stars in Ophiuchus Four New Variable Stars in Ophiuchus

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011oejv..135....1f&link_type=abstract

Open European Journal on Variable stars, Vol. 135, p. 1 (2011)

Physics

Scientific paper

Four new variable stars were discovered by serendipity in the Ophiuchus constellation during photometric analysis of the NEO Asteroid (1988 PA), pictures taken in July 2010 from A81 Balzaretto Observatory in Rome. Based on their light curves and colour indexes, the stars were classified in their variable class and registered in the Variable Star Index (VSX) hosted in the AAVSO web site, respectively as one eclipsing variable EA-type or short period eclipsing subgroup of RS CVn-type (UCAC3 196-166827), identified as the optical counterpart of 1RXS J180755.7+074717 X-ray source, two eclipsing binaries EW-type (UCAC3 196-166958 and UCAC3 196-167279) and one very likely as pulsating variable High Amplitude δ,, Scuti type (HADS) or SX Phe (UCAC3 196-167073).

Affiliated with

Also associated with

No associations

Rating

Four New Variable Stars in Ophiuchus does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Four New Variable Stars in Ophiuchus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Four New Variable Stars in Ophiuchus will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1401544