The interacting galaxy pair NGC 4485 and NGC 4490 - Star formation and the interstellar medium

Details The interacting galaxy pair NGC 4485 and NGC 4490 - Star formation and the interstellar medium The interacting galaxy pair NGC 4485 and NGC 4490 - Star formation and the interstellar medium

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989apj...339..803t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 339, April 15, 1989, p. 803-811.

Astronomy and Astrophysics

Astrophysics

18

Astronomical Spectroscopy, Interacting Galaxies, Interstellar Matter, Star Formation, Cosmic Dust, Emission Spectra, H Alpha Line, Infrared Spectra, Spectral Energy Distribution, Visible Spectrum

Scientific paper

The 100- and 160-micron continuum emission from cool dust in the
interacting gas-rich pair of galaxies, NGC 4490 and NGC 4485, was
mapped. Visual continuum and H-alpha images of the pair were obtained.
The state of the interstellar medium and the rate and efficiency of star
formation are investigated.

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