Anomalous strength of the 2200 A feature in Cassiopeia-Taurus association

Details Anomalous strength of the 2200 A feature in Cassiopeia-Taurus association Anomalous strength of the 2200 A feature in Cassiopeia-Taurus association

May 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....85..302m&link_type=abstract

Astronomy and Astrophysics, vol. 85, no. 3, May 1980, p. 302-304. Research supported by the Comision Nacional de Investigacion

Astronomy and Astrophysics

Astronomy

5

B Stars, Cassiopeia Constellation, Interstellar Extinction, Star Clusters, Taurus Constellation, Ultraviolet Astronomy, Absorption Spectra, Interstellar Matter, Spectral Line Width, Stellar Spectra

Scientific paper

From a large sample of reddened stars we computed the individual
extinction curves which agree with that calculated by Nandy et
al. (1976), except for four stars which show that the extinction at
the 2200 Å feature is greater than that deduced for the rest of
stars. These four stars belong to the Cassiopeia-Taurus association.

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