Photometric reddenings of stars in emission nebulae of the Magellanic Clouds

Details Photometric reddenings of stars in emission nebulae of the Magellanic Clouds Photometric reddenings of stars in emission nebulae of the Magellanic Clouds

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..167g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 1, July 1988, p. 167-181.

Astronomy and Astrophysics

Astrophysics

13

B Stars, Magellanic Clouds, Nebulae, O Stars, Stellar Radiation, Stellar Spectrophotometry, Hertzsprung-Russell Diagram, Main Sequence Stars, Milky Way Galaxy, Supergiant Stars

Scientific paper

The authors present VBLUW observations of stars in emission nebulae of the SMC (N66, N83, N90) and the LMC (N8, N9, N11E, N23, N43, N48, N59, N84, N148, N159, N160A, N185, N186). The stellar population (colour indices, luminosities) and the extinction in the central regions of the nebulae are derived. The authors find several stars in particular in N159 and N160A, with extinctions Av > 1.5 mag. Intrinsically more luminous, hence more massive, stars, or groups of stars, are located in the regions of the highest extinction.

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