Extragalactic dust. IV - NGC 7625

Details Extragalactic dust. IV - NGC 7625 Extragalactic dust. IV - NGC 7625

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...249..327b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 249, no. 2, Sept. 1991, p. 327-336. Research supported by Israel Academy of Sc

Astronomy and Astrophysics

Astrophysics

28

Cosmic Dust, Galactic Evolution, Interstellar Matter, Spectral Bands, Star Formation, Astronomical Photometry, Interstellar Extinction

Scientific paper

A photometric study of the early-type galaxy with dust lanes NGC 7625 is presented. The apparent extinction law of the particles in the dust lanes is derived and R about 2.8, explained as dust grains that are marginally smaller than Galactic dust grains, is found. The emission characteristics of N 7625 at various spectral bands are analyzed and star formation processes therein are discussed.

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