NGC 777 is an elliptical galaxy in the constellation of Triangulum. It was discovered by William Herschel on September 12, 1784. It has a weak active nucleus of type Seyfert 2 or LINER 2,[4] implying that the central region is obscured. When observed in radio waves the galaxy has a bright nucleus from which emerge small two radio jets about 18 kpc across. The jets are of Fanaroff–Riley class I.[5] It may be an outlying member of galaxy cluster Abell 262.[6]
↑Ho, Luis C.; Filippenko, Alexei V.; Sargent, Wallace L. W. (1997). "A Search for "Dwarf" Seyfert Nuclei. III. Spectroscopic Parameters and Properties of the Host Galaxies". The Astrophysical Journal Supplement Series112 (2): 315–390. doi:10.1086/313041. Bibcode: 1997ApJS..112..315H.
↑Capetti, A.; Brienza, M.; Balmaverde, B.; Best, P. N.; Baldi, R. D.; Drabent, A.; Gürkan, G.; Rottgering, H. J. A. et al. (April 2022). "The LOFAR view of giant, early-type galaxies: Radio emission from active nuclei and star formation". Astronomy & Astrophysics660: A93. doi:10.1051/0004-6361/202142911. Bibcode: 2022A&A...660A..93C.
↑Faber, S. M. (1989). "Spectroscopy and Photometry of Elliptical Galaxies. VI. Sample Selection and Data Summary". The Astrophysical Journal Supplement Series69: 763–808. doi:10.1086/191327. Bibcode: 1989ApJS...69..763F.