Stellar spectroscopy in the infrared at high spectral resolution

Details Stellar spectroscopy in the infrared at high spectral resolution Stellar spectroscopy in the infrared at high spectral resolution

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phst..134a4001r&link_type=abstract

Physica Scripta, Volume 134, Issue , pp. 014001 (2009).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

I present aspects of infrared (IR) stellar spectroscopy at high spectral resolution, where consideration is mostly given to near-IR (1-5 μm) spectroscopy of cool stars. Discussion is presented on applying IR spectroscopy to study the origin of sulfur, the origin of the Galactic Bulge, and the 12 μm Mg I emission feature. I briefly discuss the atomic and molecular data requirements of stellar astrophysicists.

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