Infrared laboratory spectroscopy with astrophysical applications

Details Infrared laboratory spectroscopy with astrophysical applications Infrared laboratory spectroscopy with astrophysical applications

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009phst..134a4009n&link_type=abstract

Physica Scripta, Volume 134, Issue , pp. 014009 (2009).

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

The infrared (IR) atomic spectral lines that can be observed in laboratory and astrophysical spectra depend both on the atomic structure and the physical conditions in which the atoms reside. This is a brief review of IR laboratory spectroscopy, discussing which lines in the wavelength interval 1-5 μm can be expected to be seen in different astrophysical sources.

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