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NGC 4565

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Revision as of 08:56, 11 June 2021 by The Space Enthusiast (talk | contribs) (Modified slightly)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff) Edge-on spiral galaxy in the constellation Coma Berenices
NGC 4565
NGC 4565 by Ken Crawford
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12 36 20.8
Declination+25° 59′ 16″
Redshift0.004103
Heliocentric radial velocity1230 ± 5 km/s
Distance42.7 ± 12 Mly (13.1 ± 3.7 Mpc)
53 ± 4 Mly (16.2 ± 1.3 Mpc)
Apparent magnitude (V)10.42
Characteristics
TypeSA(s)b?
Apparent size (V)15′.90 × 1′.85
Other designations
UGC 7772, PGC 42038, 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. 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. First recorded in 1785 by William Herschel, it is a prominent example of an edge-on spiral galaxy.

Characteristics

NGC 4565 is a giant spiral galaxy more luminous than the Andromeda Galaxy. 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. 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.

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

NGC 4565 is one of the brightest member galaxies of the Coma I Group.

This edge-on galaxy exhibits a slightly warped and extended disk under deep optical surveys- likely due to ongoing interactions with neighboring satellite galaxies or other galaxies in the Coma I group. The GALEX image shown below highlights the slight warp at the edge of the disc more clearly than other surveys.

Gallery

References

  1. ^ "Results for NGC 4565". NASA/IPAC Extragalactic Database. Retrieved 2006-10-12.
  2. ^ "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. S2CID 551714.
  4. "NGC4565 at". apod.nasa.gov.
  5. Spiral Galaxy NGC 4565 at http://www.eso.org/public/images/eso0525a/
  6. ^ 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. ^ "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.

External links


Astronomical catalogs
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UGC
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Caldwell catalogue
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See also
New General Catalogue 4500 to 4999
Constellation of Coma Berenices
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
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