Spectroscopy and photometry of the obscured galaxy associated with G127.11+0.54

Details Spectroscopy and photometry of the obscured galaxy associated with G127.11+0.54 Spectroscopy and photometry of the obscured galaxy associated with G127.11+0.54

Oct 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..619s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Oct.-Nov. 1979, p. 619-623.

Astronomy and Astrophysics

Astronomy

16

Astronomical Photography, Astronomical Photometry, Astronomical Spectroscopy, Elliptical Galaxies, Optical Emission Spectroscopy, Radio Galaxies, Forbidden Bands, H Alpha Line, Radial Velocity, Red Shift, Spectrophotometry

Scientific paper

Crossley reflector photographs show that Caswell's identification for the optical associated with the compact radio source centered on B127.11+0.54 is indeed a luminous obscured galaxy, similar to M87. IDS spectra show emission lines of [N II], Hα, and [S II] (in order of strength) in the red, yielding a heliocentric radial velocity of +5490 ± 90 km s-1. Our velocity and conclusions as to the extragalactic nature of the central source are in good agreement with those of Kirshner and Chevalier.

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