The novalike star TT ARIETIS - A binary system with conical accretion?

Details The novalike star TT ARIETIS - A binary system with conical accretion? The novalike star TT ARIETIS - A binary system with conical accretion?

Dec 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982sval....8..393v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 8, Dec. 1982, p. 729-733) Soviet Astronomy Letters (ISSN 0360-0327), vol. 8, Nov.-Dec.

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Line Spectra, Stellar Mass Accretion, Stellar Spectrophotometry, Light Curve, Orbital Elements, Radial Velocity, Shock Waves, Spectral Line Width, Stellar Luminosity, Velocity Distribution

Scientific paper

In October 1980, during its low-luminosity state, spectrograms of the
novalike star TT Ari were obtained with the 6 m telescope. Between
phases 0.5 and 0.6 of the 3h 12m orbital period the radial velocities
jump abruptly, perhaps because the line of sight crosses a conical shock
generated by accretion in this binary system.

Affiliated with

Also associated with

No associations

Rating

The novalike star TT ARIETIS - A binary system with conical accretion? 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 The novalike star TT ARIETIS - A binary system with conical accretion?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The novalike star TT ARIETIS - A binary system with conical accretion? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-932413