The spectral features and the chemical abundances of CP2 and HgMn stars derived from high dispersion spectra

Details The spectral features and the chemical abundances of CP2 and HgMn stars derived from high dispersion spectra The spectral features and the chemical abundances of CP2 and HgMn stars derived from high dispersion spectra

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asthe..96..383n&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 96, No. 7, p. 383 - 391 (2003)

Astronomy and Astrophysics

Astronomy

1

Chemically Peculiar Stars, Hg-Mn Stars, Spectra, Element Abundances

Scientific paper

The complex spectral features and the results of recent studies for chemically peculiar (CP) stars are reviewed with the emphasis on the magnetic peculiar and mercury-manganese stars. We stress that modern analyses using high dispersion spectrographs including HDS (High Dispersion Spectrograph) at the Subaru telescope (NAOJ) and recent atomic data have revealed the presence of emission lines of some metals on mercury-manganese stars and the complex spectra on magnetic CP stars to be partly due to the absorption lines of second ionized rare earths.

Affiliated with

Also associated with

No associations

Rating

The spectral features and the chemical abundances of CP2 and HgMn stars derived from high dispersion spectra 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 spectral features and the chemical abundances of CP2 and HgMn stars derived from high dispersion spectra, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The spectral features and the chemical abundances of CP2 and HgMn stars derived from high dispersion spectra will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1465915