Cannabaceae

NGC 2715
Pan-STARRS image of NGC 2715
Observation data (J2000 epoch)
ConstellationCamelopardalis
Right ascension09h 08m 06.196s[1]
Declination+78° 05′ 06.57″[1]
Redshift0.004466[2]
Heliocentric radial velocity1339 km/s[2]
Distance67.35 ± 10.92 Mly (20.650 ± 3.347 Mpc)[2]
Group or clusterNGC 2715 group[3]
Apparent magnitude (V)11.56[4]
Apparent magnitude (B)11.79[4]
Characteristics
TypeSAB(rs)c[2]
Size98,000 ly (30,100 pc)[2][note 1]
Apparent size (V)4.9 × 1.7[2]
Other designations
UGC 4759, MGC+13-07-015, PGC 25676[5]

NGC 2715 is an intermediate spiral galaxy in the constellation Camelopardalis. It was discovered in 1871 by Alphonse Borrelly.[6] It is an intermediate spiral galaxy that is 4.9 arcminutes wide.[2]

SN 1987M, a supernova, was discovered in NGC 2715.[7]

References

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  1. ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  2. ^ a b c d e f g "NED results for object NGC 2509". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. Retrieved 9 August 2017.
  3. ^ Tully, R. Brent; Courtois, Hélène M.; Dolphin, Andrew E.; Fisher, J. Richard; Héraudeau, Philippe; Jacobs, Bradley A.; Karachentsev, Igor D.; Makarov, Dmitry; Makarova, Lidia; Mitronova, Sofia; Rizzi, Luca; Shaya, Edward J.; Sorce, Jenny G.; Wu, Po-Feng (2013). "Cosmicflows-2: The Data". The Astronomical Journal. 146 (4): 86. arXiv:1307.7213. Bibcode:2013AJ....146...86T. doi:10.1088/0004-6256/146/4/86. S2CID 118494842.
  4. ^ a b Héraudeau, Philippe; Simien, François (1996). "Optical and I-band surface photometry of spiral galaxies. I. The data". Astronomy and Astrophysics Supplement. 118: 111–155. Bibcode:1996A&AS..118..111H. doi:10.1051/aas:1996185.
  5. ^ "NGC 2715". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 9 August 2017.
  6. ^ "New General Catalog Objects: NGC 2700 - 2749". cseligman.com. Retrieved 9 August 2017.
  7. ^ Szeidl, Béla; Lovas, Miklós (1987). "Supernova 1987M in NGC 2715". IAU Circular. 4451 (4451): 1. Bibcode:1987IAUC.4451....1S.

Notes

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  1. ^ RC3 D0 (blue) values used.
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One thought on “Cannabaceae

  1. Well, that’s interesting to know that Psilotum nudum are known as whisk ferns. Psilotum nudum is the commoner species of the two. While the P. flaccidum is a rare species and is found in the tropical islands. Both the species are usually epiphytic in habit and grow upon tree ferns. These species may also be terrestrial and grow in humus or in the crevices of the rocks.
    View the detailed Guide of Psilotum nudum: Detailed Study Of Psilotum Nudum (Whisk Fern), Classification, Anatomy, Reproduction

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