The dumb-bell galaxy NGC 750/751

Details The dumb-bell galaxy NGC 750/751 The dumb-bell galaxy NGC 750/751

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ap%26ss.170..311d&link_type=abstract

(IAU, European Regional Astronomy Meeting, 11th, La Laguna, Spain, July 3-8, 1989) Astrophysics and Space Science (ISSN 0004-640

Astronomy and Astrophysics

Astrophysics

Astronomical Photometry, Brightness, Charge Coupled Devices, Galactic Structure, Metallicity, Cosmic Dust, Elliptical Galaxies, Isophotes, Stellar Evolution, Stellar Luminosity

Scientific paper

A quantitative analysis of this system from BVR CCD photometry and long slit spectroscopy is presented. The results indicate that they constitute a physically interacting system. The presence of a dust structure along the line joining the nuclei and the members show isophotal distortion is detected, indicating a nonelliptical component, which is also seen in the surface brightness profiles.

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