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Atomic and molecular data for optical stellar spectroscopy

Heiter, U; Lind, K; Asplund, Martin; Barklem, Paul S; Bergemann, Maria; Magrini, Laura; Masseron, Thomas; Mikolaitis, S; Pickering, J C; Ruffoni, M P

Description

High-precision spectroscopy of large stellar samples plays a crucial role for several topical issues in astrophysics. Examples include studying the chemical structure and evolution of the Milky Way Galaxy, tracing the origin of chemical elements, and characterizing planetary host stars. Data are accumulating from instruments that obtain high-quality spectra of stars in the ultraviolet, optical and infrared wavelength regions on a routine basis. These instruments are located at ground-based 2-10...[Show more]

CollectionsANU Research Publications
Date published: 2015
Type: Journal article
URI: http://hdl.handle.net/1885/70023
Source: Physica Scripta
DOI: 10.1088/0031-8949/90/5/054010

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