Extinction towards 30 Doradus (LMC) derived from common upper level P(gamma)/H(delta) and P(delta)/H(epsilon) line ratios

Details Extinction towards 30 Doradus (LMC) derived from common upper level P(gamma)/H(delta) and P(delta)/H(epsilon) line ratios Extinction towards 30 Doradus (LMC) derived from common upper level P(gamma)/H(delta) and P(delta)/H(epsilon) line ratios

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...251..575g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 251, no. 2, Nov. 1991, p. 575-580.

Astronomy and Astrophysics

Astrophysics

4

Balmer Series, Interstellar Extinction, Line Spectra, Nebulae, Charge Coupled Devices, Emission Spectra, Magellanic Clouds

Scientific paper

Spectrophotometric measurements of a slit section across the 30 Dor nebula in the LMC are used to derive the absolute magnitude and the spatial variation of the extinction toward the nebula. Several combinations of Paschen-Balmer lines are used, in particular the corresponding multiplet lines P(gamma)-H(delta) and P(delta)-H(epsilon), which originate from the same upper atomic level.

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