NGC 57 explained
Upright: | 1.35 |
NGC 57 |
Epoch: | J2000 |
Type: | E[1] |
Z: | 0.018146 |
Dist Ly: | 243 Mly[2] |
Appmag V: | 11.8[3] |
Appmag B: | 12.8 |
Size V: | 2.2 × 1.9 |
Constellation Name: | Pisces |
Names: | UGC 145, PGC 1037 |
NGC 57 is an elliptical galaxy in the constellation Pisces.[3] It was discovered on 8 October 1784 by astronomer William Herschel.[4]
SN 2010dq
On June 3, 2010, Koichi Itagaki detected a magnitude 17 supernova 17" west and 1" south of the center of NGC 57 at coordinates 00 15 29.70 +17 19 41.0: Itagaki detected the August 29th 2011 an other supernova in NGC 57, 2011fp, with magnitude 17,9.[5] [6]
See also
External links
Notes and References
- Web site: NASA/IPAC Extragalactic Database . Results for NGC 57 . 2006-12-22 .
- An object's distance from Earth can be determined using Hubble's law: v=Ho is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity and v=Ho
- Web site: Revised NGC Data for NGC 57. spider.seds.org. 2017-12-18.
- Web site: New General Catalog Objects: NGC 50 - 99. cseligman.com. en-US. 2017-12-18.
- Web site: Latest Supernovae . supernovae.net (International Supernovae Network) . David Bishop . 2010-06-04.
- http://www.cbat.eps.harvard.edu/cbet/002800/CBET002820.txt Cbet 2820 del 20 settembre 2011