Rotation and Chemical Abundances of Magnetic Ap/Bp Members of the Open Cluster NGC 6475

Details Rotation and Chemical Abundances of Magnetic Ap/Bp Members of the Open Cluster NGC 6475 Rotation and Chemical Abundances of Magnetic Ap/Bp Members of the Open Cluster NGC 6475

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jrasc..99t.137f&link_type=abstract

Journal of the Royal Astronomical Society of Canada, Vol. 99, No. 4, p.137

Astronomy and Astrophysics

Astronomy

Scientific paper

Membership in the open cluster NGC 6475 (age = 220 Myr) has been confirmed for the four magnetic Ap/Bp stars HD 162305, HD 162576, HD 162725, and HD 320764. High-resolution spectra of the Ap stars, obtained within the context of the POP project with the UVES spectrograph at the ESO-VLT, were modelled in detail using LTE spectrum synthesis. Based on direct comparison of the observed and calculated line profiles, projected rotational velocities and photospheric abundances of 11 elements have been derived.

Affiliated with

Also associated with

No associations

Rating

Rotation and Chemical Abundances of Magnetic Ap/Bp Members of the Open Cluster NGC 6475 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 Rotation and Chemical Abundances of Magnetic Ap/Bp Members of the Open Cluster NGC 6475, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Rotation and Chemical Abundances of Magnetic Ap/Bp Members of the Open Cluster NGC 6475 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-856687