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Stellar spectroscopy in the infrared at high spectral resolution
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Astronomy and Space Physics.
2009 (English)In: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. T134, 014001- p.Article in journal (Refereed) Published
Abstract [en]

I present aspects of infrared (IR) stellar spectroscopy at high spectral resolution, where consideration is mostly given to near-IR (1-5 mu m) 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 mu m Mg I emission feature. I briefly discuss the atomic and molecular data requirements of stellar astrophysicists.

Place, publisher, year, edition, pages
2009. Vol. T134, 014001- p.
National Category
Physical Sciences
URN: urn:nbn:se:uu:diva-148810DOI: 10.1088/0031-8949/2009/T134/014001ISI: 000267612800002OAI: oai:DiVA.org:uu-148810DiVA: diva2:403365
Available from: 2011-03-12 Created: 2011-03-10 Last updated: 2011-03-12Bibliographically approved

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