X-ray coronae from dynamos in young Ae/Be stars

Details X-ray coronae from dynamos in young Ae/Be stars X-ray coronae from dynamos in young Ae/Be stars

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.272..528t&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 272, Issue 3, pp. 528-530.

Astronomy and Astrophysics

Astronomy

55

Magnetic Fields-, Stars: Coronae, Stars: Emission-Line, Be, X-Rays: Stars

Scientific paper

Recent observations by Zinnecker & Preibisch indicate that young
Ae/Be stars are significant X-ray emitters. Here we suggest that this
X-ray emission comes from a corona which is heated by magnetic activity.
We argue that dynamo activity can be sustained in these predominantly
radiative stars by tapping the initial stellar differential rotation.

Affiliated with

Also associated with

No associations

Rating

X-ray coronae from dynamos in young Ae/Be 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 X-ray coronae from dynamos in young Ae/Be stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray coronae from dynamos in young Ae/Be stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1635535