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MCG +07-33-027

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Isolated spiral galaxy in the constellation Hercules
MCG +07-33-027
Starburst galaxy MCG +07-33-027 as imaged by the Hubble Space Telescope.
Observation data (J2000 epoch)
ConstellationHercules
Right ascension16 02 16.6
Declination42° 55′ 01″
Redshift0.024486/7341 km/s
Distance329,462,000 ly
Apparent magnitude (V)14.5
Characteristics
TypeSa
Size~104,057.8 ly (estimated)
Apparent size (V)0.86' x 0.74
Other designations
PGC 56779

MCG +07-33-027 is an isolated spiral galaxy located about 330 million light-years away in the constellation Hercules. It has a very high rate of star formation which would make it a starburst galaxy. Normally, starburst galaxies are triggered by the collision of another galaxy. However most galaxies are in groups or clusters, while MCG +07-33-027 is solitary. Therefore, the cause of the starburst was not due to a collision or by the passing of a nearby galaxy and so the cause of the activity remains unknown.

On April 2, 2005, SN 2005bk, a supernova (type Ic, mag. 18) was discovered in MCG +07-33-027.

See also

References

  1. ^ "NASA/IPAC Extragalactic Database". Results for MCG +07-33-027. Retrieved 2017-07-26.
  2. ^ "A lonely birthplace". www.spacetelescope.org. Retrieved 2017-07-27.
  3. "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2017-07-27.
  4. "Principal Galaxy Catalog (PGC) Objects 56500 to 56999". cseligman.com. Retrieved 2017-07-27.
  5. "IAUC 8512: 2005bk; 2005bl; 9P". www.cbat.eps.harvard.edu. Retrieved 2017-07-27.
  6. Transient Name Server entry for SN 2005bk. Retrieved 3 August 2024.

External links

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