CCD Spectrophotometry of Dwarf Novae

Details CCD Spectrophotometry of Dwarf Novae CCD Spectrophotometry of Dwarf Novae

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998larm.confe..29c&link_type=abstract

"IX Latin American Regional IAU Meeting, "Focal Points in Latin American Astronomy", held in Tonantzintla, Mexico, Nov 9-13, 199

Astronomy and Astrophysics

Astronomy

Scientific paper

We present spectroscopic observations of the dwarf novae KT Per, TZ Per and TT Boo. For the first two objects we have measured radial velocities that allow us to improve their orbital periods: 0.161825792+/-0.000000006 days, for KT Per and 0.262719+/-0.000001 days for TZ Per. The spectra of the faint dwarf nova TT Boo at times show a doble profile in the Hα emission line. From this line we find an orbital period of 0.29123 +/- 0.0004 days, a value much larger than that expected from the superhump frequencies reported in the literature.

Affiliated with

Also associated with

No associations

Rating

CCD Spectrophotometry of Dwarf Novae 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 CCD Spectrophotometry of Dwarf Novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CCD Spectrophotometry of Dwarf Novae will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-802424