Infrared spectroscopy in astronomy

Details Infrared spectroscopy in astronomy Infrared spectroscopy in astronomy

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981spie..280...29h&link_type=abstract

In: Infrared astronomy - Scientific/military thrusts and instrumentation; Proceedings of the Meeting, Washington, DC, April 21,

Astronomy and Astrophysics

Astronomy

Astronomical Spectroscopy, Infrared Astronomy, Infrared Instruments, Infrared Spectroscopy, Resolution, Background Radiation, Design Analysis, Radiant Flux Density, Thermal Emission

Scientific paper

The use of infrared spectroscopy in astronomy has increased dramatically in the past ten years. The broad design considerations are discussed in terms of wavelength coverage and resolution. Three rough resolution ranges, lambda/Delta lambda of approximately 100, 1000 and 10,000, are identified in which various types of astronomical problems can be studied. Numerous existing systems are briefly discussed and references are given to more complete descriptions.

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