Spectral Observations of the Novalike Star TT Ari

Details Spectral Observations of the Novalike Star TT Ari Spectral Observations of the Novalike Star TT Ari

Oct 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap.....47..462m&link_type=abstract

Astrophysics (English translation of Astrofizika), v. 47, Issue 4, p. 462-471 (2004).

Astronomy and Astrophysics

Astrophysics

Stars, Novalike: Stars, Individual, Tt Ari, Stars - Novalike - Stars - Individual - Tt Ari

Scientific paper

Spectral observations of the novalike star TT Ari at the Byurakan Observatory in September 2001 are reported. In most cases these results are in good agreement with earlier observational data. Some interesting differences from the earlier results were obtained, in particular the absence of emission and the presence of very weak absorption in the H line. Another interesting difference that was recorded is the absence of an anti-P Cygni H line profile along with rapid variations in the P Cygni profile during our observations.

Affiliated with

Also associated with

No associations

Rating

Spectral Observations of the Novalike Star TT Ari 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 Spectral Observations of the Novalike Star TT Ari, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Spectral Observations of the Novalike Star TT Ari will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-897028