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NGC 4395 is a nearby low surface brightness spiral galaxy located about 14 million light-years (or 4.3 Mpc) from Earth in the constellation Canes Venatici.[4] The nucleus of NGC 4395 is active and the galaxy is classified as a Seyfert Type I known for its very low-mass supermassive black hole.[5]
^Cite error: The named reference NSOG was invoked but never defined (see the help page).
^Thim, F.; Hoessel, J. G.; Saha, A.; Claver, J.; Dolphin, A.; Tammann, G. A. (April 2004). "Cepheids and Long-Period Variables in NGC 4395". The Astronomical Journal. 127 (4): 2322–2343. arXiv:astro-ph/0401558. Bibcode:2004AJ....127.2322T. doi:10.1086/382244. ISSN 0004-6256. S2CID 14631171.
^Filippenko, Alexei V.; Ho, Luis C. (25 March 2003). "A Low-Mass Central Black Hole in the Bulgeless Seyfert 1 Galaxy NGC 4395". The Astrophysical Journal Letters. 588 (1): L13. arXiv:astro-ph/0303429. Bibcode:2003ApJ...588L..13F. doi:10.1086/375361. S2CID 14411746. Retrieved 20 August 2020.
NGC4395 is a nearby low surface brightness spiral galaxy located about 14 million light-years (or 4.3 Mpc) from Earth in the constellation Canes Venatici...
October 2005). "Multiwavelength Monitoring of the Dwarf Seyfert 1 Galaxy NGC4395. I. A Reverberation-Based Measurement of the Black Hole Mass". The Astrophysical...
galaxies M31 and M32, and a few galaxies beyond the Local Group, e.g. NGC4395. In these galaxies, the mean square (or root mean square) velocities of...
galaxies M31 and M32, and a few galaxies beyond the Local Group, such as NGC4395. In these galaxies, the root mean square (or rms) velocities of the stars...
NGC 300 is an "SA(s)d" NGC 45 SAdm SAdm can also be considered a type of unbarred Magellanic spiral NGC 45 is an "SA(s)dm" NGC4395 SAm SAm is a type of...
holes in its center NGC4395, an example of a low surface brightness galaxy with an intermediate-mass black hole in its center NGC 4725, one of the closest...
identified with the NSC. A few galaxies, for instance the Milky Way and NGC4395, are known to contain both a SBH and a NSC. Although this is suggestive...
created from the Nearby Optical Galaxy sample of Giuricin et al. Additionally, NGC 4105 and DDO 169 are frequently but not consistently identified as members...
NGC 4036 is the New General Catalogue identifier for a lenticular galaxy in the northern circumpolar constellation of Ursa Major. In the Carnegie Atlas...
NGC 820 is a spiral galaxy located in the constellation Aries about 210 million light-years from the Milky Way. It was discovered by British astronomer...
NGC 4041 is the New General Catalogue identifier for a spiral galaxy in the northern circumpolar constellation of Ursa Major. It is located an estimated...
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