Jump to content

NGC 2441

Coordinates: Sky map 07h 51m 54.772s, +73° 00′ 56.42″
From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by Tom.Reding (talk | contribs) at 18:31, 27 February 2018 (Fix Category:Pages using deprecated image syntax; WP:GenFixes on, using AWB). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.


NGC 2441
NGC 2441 spiral galaxy taken by Hubble
Observation data (J2000 epoch)
ConstellationCamelopardalis
Right ascension07h 51m 54.772s [1]
Declination+73° 00′ 56.42″[1]
Redshift0.01157[1]
Heliocentric radial velocity3450 km/s[1]
Distance180 million ly[2]
Apparent magnitude (B)12.7[1]
Characteristics
TypeSBc[1]
Size2.633 x 1.159 arcmin[1]
Other designations
2MASX J07515477+7300564, UZC J075154.8+730055, [CHM2007] LDC 573 J075154.77+7300564, HIJASS J0751+72, MCG+12-08-015, Z 331-17, LEDA 22031, UGC 4036, Z 0746.1+7308
In this Hubble Space Telescope image of NGC 2441, supernova SN1995E is the white spot within the red circle.

NGC 2441 is a barred spiral galaxy located in the northern constellation of Camelopardalis.[2] A Type 1a supernova, SN1995E, occurred in NGC 2441, and observations suggest it may display a light echo, where light from the supernova is reflected from matter along our line of sight, making it appear to "echo" outwards from the source.[2] The diameter of the galaxy is about 130,000 light-years.

References

  1. ^ a b c d e f g "Search Results for NGC 2441". http://simbad.u-strasbg.fr/simbad/. SIMBAD. Retrieved 25 June 2014. {{cite web}}: External link in |website= (help)
  2. ^ a b c "A curious supernova in NGC 2441". ESA/Hubble Picture of the Week. ESA/Hubble. Retrieved 25 June 2014.