Dust in emission nebulae of the LMC derived from photometric reddening of stars

Details Dust in emission nebulae of the LMC derived from photometric reddening of stars Dust in emission nebulae of the LMC derived from photometric reddening of stars

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26as...85..895g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 85, no. 2, Oct. 1990, p. 895-913.

Astronomy and Astrophysics

Astrophysics

6

Cosmic Dust, Emission Spectra, Interstellar Extinction, Magellanic Clouds, Nebulae, Stellar Spectrophotometry, Balmer Series, Hertzsprung-Russell Diagram, Main Sequence Stars, Stellar Luminosity, Stellar Magnitude

Scientific paper

VBLUW photometric observations of stars in emission nebulae of the LMC are reported. The luminosities and extinctions of the stars are derived. Agreement is found between the average photometric extinctions of the nebulae and the extinctions derived from the Balmer line decrement measured by Caplan and Deharveng (1985 and 1986). The photometric extinctions are shown in the CO map of the LMC (Cohen et al., 1988).

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