Recurrent Nova T Pyx is Deviating from 1967 Eruption Light Curve

Details Recurrent Nova T Pyx is Deviating from 1967 Eruption Light Curve Recurrent Nova T Pyx is Deviating from 1967 Eruption Light Curve

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011atel.3707....1s&link_type=abstract

The Astronomer's Telegram, #3707

Astronomy and Astrophysics

Astronomy

Optical, Request For Observations, Nova

Scientific paper

We report on the light curve of the recurrent nova T Pyx, now in eruption (IAUC #9205, ATel #3549, ATel #3647). Our optical observations are made with the 0.5-m telescope at the Caisey Harlingten Observatory near San Pedro de Atacama in Chile. The V-band magnitudes were made as part of time series (with 30-second time resolution) lasting 0.9-3.6 hours on 115 nights since May 12. T Pyx was followed throughout the entire interval of solar conjunction (with T Pyx 46.4° from the Sun on August 25).

Affiliated with

Also associated with

No associations

Rating

Recurrent Nova T Pyx is Deviating from 1967 Eruption Light Curve 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 Recurrent Nova T Pyx is Deviating from 1967 Eruption Light Curve, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Recurrent Nova T Pyx is Deviating from 1967 Eruption Light Curve will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1651771