NGC 3077

NGC 3077 is a small disrupted elliptical galaxy, a member of the M81 Group, which is located in the northern constellation Ursa Major. Despite looking much like an elliptical galaxy, it is peculiar for two reasons. First, it shows wispy edges and scattered dust clouds that are probably a result of gravitational interaction with its larger neighbors, similar to the galaxy M82. Second, this galaxy has an active nucleus. This caused Carl Seyfert in 1943 to include it in his list of galaxies, which are now called Seyfert Galaxies. However, NGC 3077, though an emission line galaxy, is today no longer classified as a Seyfert galaxy.

NGC 3077
NGC 3077 by HST, 1.5′ view
Observation data (J2000 epoch)
ConstellationUrsa Major
Right ascension 10h 03m 19.1s[1]
Declination+68° 44′ 02″[1]
Redshift14 ± 4 km/s[1]
Distance12.8 ± 0.7 Mly (3.9 ± 0.2 Mpc)[2][3][4][a]
Apparent magnitude (V)10.6[1]
Characteristics
TypeI0 pec[1]
Apparent size (V)5′.4 × 4′.5[1]
Other designations
UGC 5398,[1] PGC 29146[1]

NGC 3077 was discovered by William Herschel on November 8, 1801. He remarked that "On the nF (NE) side, there is a faint ray interrupting the roundness." Admiral Smyth described it as "A bright-class round nebula; it is a lucid white, and lights up in the centre ... between these [stars,] the sky is intensely black, and shows the nebula as if floating in awful and illimitable space, at an inconceivable distance."

Distance measurements

At least two techniques have been used to measure distances to NGC 3077. The surface brightness fluctuations (SBF) distance measurement technique estimates distances to spiral galaxies based on the graininess of the appearance of their bulges. The distance measured to NGC 3077 using this technique is 13.2 ± 0.8 Mly (4.0 ± 0.2 Mpc).[2] However, NGC 3077 is close enough that the tip of the red giant branch (TRGB) method may be used to estimate its distance. The estimated distance to NGC 3077 using this technique is 12.5 ± 1.2 Mly (3.82 ± 0.38 Mpc).[3] Averaged together, these distance measurements give a distance estimate of 12.8 ± 0.7 Mly (3.9 ± 0.3 Mpc).[a]

Sources

Notes
  1. ^ average(4.0 ± 0.2,[2] 3.82 ± 0.38[3]) = ((4.0 + 3.82) / 2) ± ((0.22 + 0.382)/2)0.5 = 3.9 ± 0.3
gollark: It's a bad wrapper over modems.
gollark: Yep.
gollark: It's not an email, it's a pseudocryptocurrency.
gollark: Site-41 on CN has an APIONET interdimensional relay server rack, which frequently crashed partly due to power loss despite being connected to the site's entire generator array.
gollark: If you transmit APIONET messages on a loop from an average computer, you can easily make all the nearby repeaters crash from power failure even though they have 300RF/t of generator capacity.

References
  1. "NASA/IPAC Extragalactic Database". Results for NGC 3077. Retrieved 2006-12-13.
  2. J. L. Tonry; A. Dressler; J. P. Blakeslee; E. A. Ajhar; et al. (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal. 546 (2): 681–693. arXiv:astro-ph/0011223. Bibcode:2001ApJ...546..681T. doi:10.1086/318301.
  3. I. D. Karachentsev; V. E. Karachentseva; W. K. Hutchmeier; D. I. Makarov (2004). "A Catalog of Neighboring Galaxies". Astronomical Journal. 127 (4): 2031–2068. Bibcode:2004AJ....127.2031K. doi:10.1086/382905.
  4. Karachentsev, I. D.; Kashibadze, O. G. (2006). "Masses of the local group and of the M81 group estimated from distortions in the local velocity field". Astrophysics. 49 (1): 3–18. Bibcode:2006Ap.....49....3K. doi:10.1007/s10511-006-0002-6.



This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.