NGC 146 explained

NGC 146
Epoch:J2000
Constellation:Cassiopeia
Ra:[1]
Dist Ly:~10000
Dist Pc:~3000
Appmag V:9.1[2]
Age:<10 Myr
Names:Cr 5, OCl 299, C 0030+630

NGC 146 is a small open cluster in the constellation Cassiopeia. It was discovered by John Herschel in 1829 using his father's 18.7 inch reflecting telescope.[3]

Location

NGC 146 is fairly easy to locate in the sky, being half a degree away from the bright star Kappa Cassiopeiae. However, spotting the cluster itself is difficult because of its low apparent magnitude of 9.1. Its relatively high declination of about 63° means it is not visible for below 27° S.Its distance is estimated at 3030 parsecs (9880 light years),[4] but may be around 3500 pc (11000 ly) away.

Characteristics

The cluster is at most 10 million years old, as there are numerous B-type main sequence stars and pre-main-sequence stars but relatively few evolved supergiants. Among its most massive stars are two Herbig Be stars.[5]

Further reading

Notes and References

  1. Web site: NASA/IPAC Extragalactic Database . Results for NGC 0146 . 31 December 2016.
  2. NGC 146. 31 December 2016.
  3. Web site: Catalogo NGC/IC online - result for NGC 146 . July 23, 2013 . https://web.archive.org/web/20090528100240/http://www.ngcicproject.org/pubdb.htm . May 28, 2009 . dead .
  4. Web site: WEBDA page for open cluster NGC 146.
  5. Subramaniam . A. . Sahu . D. K. . Sagar . R. . Vijitha . P. . NGC 146: a young open cluster with a Herbig Be star and intermediate mass pre-main sequence stars . Astronomy and Astrophysics . September 2005 . 440 . 2 . 511‐522 . 10.1051/0004-6361:20052683 . astro-ph/0505314 . 2005A&A...440..511S . 14909422 .