Walraven photometry of WX Hyi (Kuulkers+ 1991)

Details Walraven photometry of WX Hyi (Kuulkers+ 1991) Walraven photometry of WX Hyi (Kuulkers+ 1991)

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ycat..32420401k&link_type=abstract

VizieR On-line Data Catalog: J/A+A/242/401. Originally published in: 1991A&A...242..401K

Physics

Stars: Variable, Photometry: Vbluw

Scientific paper

The SU UMa-type dwarf nova WX Hyi was observed in the 5 passbands VBLUW
(544, 430, 384, 362 and 324nm) during 15 nights on the 90cm telescope at
ESO (La Silla), between July and November 1988, with an integration time
of 16s. (1 data file).

Affiliated with

Also associated with

No associations

Rating

Walraven photometry of WX Hyi (Kuulkers+ 1991) 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 Walraven photometry of WX Hyi (Kuulkers+ 1991), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Walraven photometry of WX Hyi (Kuulkers+ 1991) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1185337