Optical extinction in HII regions and nearby bright galaxies

Details Optical extinction in HII regions and nearby bright galaxies Optical extinction in HII regions and nearby bright galaxies

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992iraj...20..191c&link_type=abstract

(Astronomical Science Group of Ireland, Meeting, Regional Technical College, Cork, Republic of Ireland, Sept. 14, 1990) Irish As

Astronomy and Astrophysics

Astronomy

Active Galaxies, Cosmic Dust, H Ii Regions, Interstellar Extinction, Astronomical Observatories, Charge Coupled Devices, Line Spectra, Near Infrared Radiation, Near Ultraviolet Radiation

Scientific paper

Observations with the 1.5 m telescope at ESO, Chile, and the 4.2 m WHT at RGO, La Palma, of galactic HII regions and three galaxies were made to evaluate the potential for Aupsilon determination, using pairs of lines from transitions from common upper levels, and separated by a large wavelength interval. Spectral lines from the near UV to the near IR are shown to be accessible with modern blue-coated CCD detectors.

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