Stellar winds in the young galactic cluster NGC 6530

Details Stellar winds in the young galactic cluster NGC 6530 Stellar winds in the young galactic cluster NGC 6530

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984nascp2349..223b&link_type=abstract

In NASA. Goddard Space Flight Center Future of Ultraviolet Astronomy Based on Six Years of IUE Res. p 223-226 (SEE N85-20961 1

Astronomy and Astrophysics

Astronomy

1

Ionization, O Stars, Stellar Temperature, Stellar Winds, Galactic Clusters, Iue, Main Sequence Stars, Stellar Luminosity, Ultraviolet Spectra

Scientific paper

The authors have studied line profiles for O stars on or close to the
main sequence in the young galactic cluster NGC 6530. P Cygni profiles
are seen for Teff > 36000K. Different stars show, however,
different lines and different outflow velocities. The degree of
ionization in the wind appears to depend on Teff.

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