Non-LTE models of accretion disks of UX Ori type stars.

Details Non-LTE models of accretion disks of UX Ori type stars. Non-LTE models of accretion disks of UX Ori type stars.

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999afz....42...75t&link_type=abstract

Astrofizika, Tom 42, Vyp. 1, p. 75 - 88

Astronomy and Astrophysics

Astronomy

7

Circumstellar Disks: Variables, Circumstellar Disks: Magnetic Fields, Circumstellar Disks: Non-Lte Models

Scientific paper

The mass accretion rate has been estimated; it ranges from M˙α = 10-8 to 10-9Msunyr-1. The gas temperature in this region is about 10000 K. In the close vicinity of the star there exists the hotter region with the temperature of more than 15000 K where the line of the neutral helium 5876 Å observed in the spectra of these stars arises. This region has a small geometrical depth, covers a small part of the visible stellar disk and, apparently, represents places where accreting gas contacts the star. Low values of the rotation velocity in this region (150 - 200 km/s) implies the presence of the magnetic field strong enough to extinguish the rapid rotation of the stream. The magnetic strength in this region is about 150 Gs.

Affiliated with

Also associated with

No associations

Rating

Non-LTE models of accretion disks of UX Ori type stars. 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 Non-LTE models of accretion disks of UX Ori type stars., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-LTE models of accretion disks of UX Ori type stars. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1028133