Elemental abundance analysis of HR 8216 (Caliskan, 2005)

Details Elemental abundance analysis of HR 8216 (Caliskan, 2005) Elemental abundance analysis of HR 8216 (Caliskan, 2005)

Sep 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003ycat..73561256c&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/356/1256. Originally published in: 2005MNRAS.356.1256C

Computer Science

Graphics

Stars: Peculiar, Abundances: Peculiar

Scientific paper

We have performed the abundance analysis of the cool magnetic CP star HR 8216 (=HD 204411) using 2.4{AA}/mm Dominion Astrophysical Observatory Reticon exposures covering ll 3830-4770{AA} with a typical signal-to-noise ratio of 200. The spectrograms were measured interactively with the graphics computer program REDUCE. We performed a fine analysis with an ATLAS9 metal-rich model atmosphere whose predictions best matched the optical region fluxes and the Hg profile. HR 8216's anomalies are primarily an enhancement of many iron peak elements with the rare earths elements much less enhanced than for many similar cool magnetic CP stars .Using the results of the fine analysis we synthetized the spectrum. Comparison with the observed spectrum showed that agreement is better.
(1 data file).

Affiliated with

Also associated with

No associations

Rating

Elemental abundance analysis of HR 8216 (Caliskan, 2005) 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 Elemental abundance analysis of HR 8216 (Caliskan, 2005), we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Elemental abundance analysis of HR 8216 (Caliskan, 2005) will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1090668