Interstellar Gas and Dust Absorptions Near NGC 6530

Details Interstellar Gas and Dust Absorptions Near NGC 6530 Interstellar Gas and Dust Absorptions Near NGC 6530

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984iue..prop.1772b&link_type=abstract

IUE Proposal ID #IEGEB

Physics

Scientific paper

In our study of the extinction law for 0 and early B stars in the young galactic clusters NGC 6530 we found a rather strong dependence of extinction on T(eff) (see Fig. 1). Since the highest temperature stars are also farthest away from the center of the cluster (see Fig. 2) this may also mean that the extinction law changes with distance from the cluster center. We want to study which is the true correlation by studying stars with the same T(eff) but at different distances from the Cluster center. We also want to study the interstellar gas, which is concentrated near the Cluster in order to see whether the gas properties change in a systematic way in accordance with the observed changes in the extinction law.

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