Jump to content

NGC 4565

Coordinates: Sky map 12h 36m 20.8s, +25° 59′ 16″
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by UnaToFiAN-1 (talk | contribs) at 05:09, 25 October 2019 (→‎External links: +{{Coma Berenices}}). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

NGC 4565
NGC 4565 or Needle Galaxy by Ken Crawford
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12h 36m 20.8s[1]
Declination+25° 59′ 16″[1]
Redshift0.004103[1]
Heliocentric radial velocity1230 ± 5 km/s[1]
Distance42.7 ± 12 Mly (13.1 ± 3.7 Mpc)[2]
53 ± 4 Mly (16.2 ± 1.3 Mpc)[3]
Apparent magnitude (V)10.42[1]
Characteristics
TypeSA(s)b?[1]
Apparent size (V)15′.90 × 1′.85[1]
Other designations
UGC 7772,[1] PGC 42038,[1] Caldwell 38

NGC 4565 (also known as the Needle Galaxy or Caldwell 38) is an edge-on spiral galaxy about 30 to 50 million light-years away in the constellation Coma Berenices.[2] It lies close to the North Galactic Pole and has a visual magnitude of approximately 10. It is known as the Needle Galaxy for its narrow profile.[4] First recorded in 1785 by William Herschel, it is a prominent example of an edge-on spiral galaxy.[5]

Characteristics

NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy.[6] Much speculation exists in literature as to the nature of the central bulge. In the absence of clear-cut dynamical data on the motions of stars in the bulge, the photometric data alone cannot adjudge among various options put forth. However, its exponential shape suggested that it is a barred spiral galaxy.[7] Studies with the help of the Spitzer Space Telescope not only confirmed the presence of a central bar but also showed a pseudobulge within it as well as an inner ring.[8]

NGC 4565 has at least two satellite galaxies, one of which is interacting with it.[9] It has a population of roughly 240 globular clusters, more than the Milky Way.[6]

NGC 4565 is one of the brightest[10] member galaxies of the Coma I Group.[11][10]

A detailed view of part of the disc of the spiral galaxy NGC 4565 imaged by the Hubble Space Telescope.

References

  1. ^ a b c d e f g h i "Results for NGC 4565". NASA/IPAC Extragalactic Database. Retrieved 2006-10-12.
  2. ^ a b "Distance Results for NGC 4565". NASA/IPAC Extragalactic Database. Retrieved 2010-05-02.
  3. ^ Jensen, Joseph B.; Tonry, John L.; Barris, Brian J.; Thompson, Rodger I.; et al. (February 2003). "Measuring Distances and Probing the Unresolved Stellar Populations of Galaxies Using Infrared Surface Brightness Fluctuations". Astrophysical Journal. 583 (2): 712–726. arXiv:astro-ph/0210129. Bibcode:2003ApJ...583..712J. doi:10.1086/345430.
  4. ^ "NGC4565 at". apod.nasa.gov.
  5. ^ Spiral Galaxy NGC 4565 at http://www.eso.org/public/images/eso0525a/
  6. ^ a b Globular Cluster Systems in Galaxies Beyond the Local Group
  7. ^ "Intermediate-band surface photometry of the edge-on galaxy NGC 4565". iop.org.
  8. ^ Detection of a Distinct Pseudobulge Hidden Inside the ``Box-Shaped Bulge of NGC 4565
  9. ^ HALOGAS: H I Observations and Modeling of the Nearby Edge-on Spiral Galaxy NGC 4565
  10. ^ a b "Webb Deep-Sky Society: Galaxy of the Month: NGC4565". www.webbdeepsky.com. Retrieved 2018-05-20.
  11. ^ Gregory, Stephen A.; Thompson, Laird A. (April 1977). "The Coma i Galaxy Cloud". The Astrophysical Journal. 213: 345–350. Bibcode:1977ApJ...213..345G. doi:10.1086/155160. ISSN 0004-637X.


Retrieved from "https://en.wikipedia.org/w/index.php?title=NGC_4565&oldid=922923092"