Wide metal-poor binaries BVRI photometry (Zapatero Osorio+, 2004)

Details Wide metal-poor binaries BVRI photometry (Zapatero Osorio+, 2004) Wide metal-poor binaries BVRI photometry (Zapatero Osorio+, 2004)

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ycat..34190167z&link_type=abstract

VizieR On-line Data Catalog: J/A+A/419/167. Originally published in: 2004A&A...419..167Z

Astronomy and Astrophysics

Astronomy

Stars: Double And Multiple, Photometry: Ubvri

Scientific paper

Observing dates, differential photometry and astrometry (rho and position angle) of companion candidates around 473 nearby, low-metallicity G- to M-type stars are provided in the Table. The target stars were mainly taken from the Carney-Latham surveys. Also provided are exposure times, the FWHM of the CCD images, and the telescope used for collecting the observations. The last column contains a flag indicating whether the candidate is a confirmed physical companion.
(2 data files).

Affiliated with

Also associated with

No associations

Rating

Wide metal-poor binaries BVRI photometry (Zapatero Osorio+, 2004) 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 Wide metal-poor binaries BVRI photometry (Zapatero Osorio+, 2004), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Wide metal-poor binaries BVRI photometry (Zapatero Osorio+, 2004) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1461446