The spin pulse of the intermediate polar V1062 Tauri

Details The spin pulse of the intermediate polar V1062 Tauri The spin pulse of the intermediate polar V1062 Tauri

Jul 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002a%26a...389..904h&link_type=abstract

Astronomy and Astrophysics, v.389, p.904-907 (2002)

Astronomy and Astrophysics

Astrophysics

7

Accretion, Accretion Disks, Stars: Individual: V1062 Tau, Novae, Cataclysmic Variables, Binaries: Close, X-Rays: Stars.

Scientific paper

We combine ASCA and RXTE data of V1062 Tau to confirm the presence of a
62-min X-ray pulsation. We show that the pulsation is caused largely by
the variation of dense partial absorption, in keeping with current
models of accretion onto magnetic white dwarfs. Further parametrisation
of the spin pulse is, however, hampered by ambiguities in the models.

Affiliated with

Also associated with

No associations

Rating

The spin pulse of the intermediate polar V1062 Tauri 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 spin pulse of the intermediate polar V1062 Tauri, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spin pulse of the intermediate polar V1062 Tauri will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-958955