NGC 5614: Difference between revisions

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| constellation name = [[Boötes]]
| constellation name = [[Boötes]]
| notes = NGC 5615 superimposed, plume, paired with NGC 5613.
| notes = NGC 5615 superimposed, plume, paired with NGC 5613.
| names = [[General Catalogue|GC]] 3880, [[h]] 1804, [[H]] 2.420, [[Arp]] 178 (with NGC 5613, 5615), [[Uppsala General Catalogue|UGC]] 9226, [[Morphological Catalogue of Galaxies|MCG]]+06-32-022, [[PGC]] 51439, [[H II]]-420, [[CGCG]] 192.014, [[Atlas of Interacting Galaxies|VV]] 77, [[IRAS]] 14220+3505, [[Atlas of Interacting Galaxies|VV]] 77a, [[Lyon-Meudon Extragalactic Database|LEDA]] 51439, [[Fritz Zwicky#Catalog_of_Galaxies_and_Clusters|Z]] 192-14, [[Atlas of Peculiar Galaxies|APG]] 178, [[2MASX]] J14240759+3451320, [[Fritz Zwicky#Catalog_of_Galaxies_and_Clusters|Z]] 1422.0+3505, [[ISOSS]] J14240+3451, [[UZC]] J142407.6+345134 }}
| names = [[General Catalogue|GC]] 3880, [[h]] 1804, [[H]] 2.420, [[Arp]] 178 (with NGC 5613, 5615), [[Uppsala General Catalogue|UGC]] 9226, [[Morphological Catalogue of Galaxies|MCG]]+06-32-022, [[Lyon-Meudon Extragalactic Database|PGC]] 51439, [[H II]]-420, [[CGCG]] 192.014, [[Atlas of Interacting Galaxies|VV]] 77, [[IRAS]] 14220+3505, [[Atlas of Interacting Galaxies|VV]] 77a, [[Lyon-Meudon Extragalactic Database|LEDA]] 51439, [[Fritz Zwicky#Catalog_of_Galaxies_and_Clusters|Z]] 192-14, [[Atlas of Peculiar Galaxies|APG]] 178, [[2MASX]] J14240759+3451320, [[Fritz Zwicky#Catalog_of_Galaxies_and_Clusters|Z]] 1422.0+3505, [[ISOSS]] J14240+3451, [[UZC]] J142407.6+345134 }}
'''NGC 5614''' is galaxy in the constellation [[Boötes]]. Interacting galaxies, NGC 5614 and [[NGC 5615]]. " '' Fairly bright, moderately large, slightly elongated E-W, 1.5' diameter. Well concentrated to a prominent 30" core. A mag 11 star lies 2.7' ESE of center. Forms a pair with N5613 2.0' N. N5615 is a knot in the halo 26" NW of the center (not seen).
'''NGC 5614''' is galaxy in the constellation [[Boötes]]. Interacting galaxies, NGC 5614 and [[NGC 5615]]. " '' Fairly bright, moderately large, slightly elongated E-W, 1.5' diameter. Well concentrated to a prominent 30" core. A mag 11 star lies 2.7' ESE of center. Forms a pair with N5613 2.0' N. N5615 is a knot in the halo 26" NW of the center (not seen).
8": faint, small, slightly elongated, small bright nucleus.'' " '''- by Steve Gottlieb'''
8": faint, small, slightly elongated, small bright nucleus.'' " '''- by Steve Gottlieb'''

Revision as of 13:28, 29 September 2008

NGC 5614
Observation data (J2000 epoch)
ConstellationBoötes
Right ascension14h 24m 07.74s
Declination+34°  51′  32.1″
Redshift0.01297 ± 0.00010
(3862 ± 30 km/s )
Distance171.9 Mly (52.73 Mpc)
Apparent magnitude (V)11.7
Characteristics
TypeSa
Apparent size (V)2.884′ × 2.344 ′
Notable featuresNGC 5615 superimposed, plume, paired with NGC 5613.
Other designations
GC 3880, h 1804, H 2.420, Arp 178 (with NGC 5613, 5615), UGC 9226, MCG+06-32-022, PGC 51439, H II-420, CGCG 192.014, VV 77, IRAS 14220+3505, VV 77a, LEDA 51439, Z 192-14, APG 178, 2MASX J14240759+3451320, Z 1422.0+3505, ISOSS J14240+3451, UZC J142407.6+345134

NGC 5614 is galaxy in the constellation Boötes. Interacting galaxies, NGC 5614 and NGC 5615. " Fairly bright, moderately large, slightly elongated E-W, 1.5' diameter. Well concentrated to a prominent 30" core. A mag 11 star lies 2.7' ESE of center. Forms a pair with N5613 2.0' N. N5615 is a knot in the halo 26" NW of the center (not seen). 8": faint, small, slightly elongated, small bright nucleus. " - by Steve Gottlieb

Historical Research Notes / Correction for NGC 5614

" NGC 5609, NGC 5613, and NGC 5615 are all companions of NGC 5614 found by LdR. In spite of the good positions in NGC, there has been some confusion over the identifications. Even if the positions were not reliable, LdR's sketch of the field, and micrometric measurements of two of the novae, would be enough to clearly identify them.

NGC 5614 and NGC 5615 have attracted recent attention as an interacting pair of galaxies. N5615 has a tidal plume streaming away from it and N5614, the clear result of the gravitational interaction. " - Dr. Harold G. Corwin, Jr.

Reference

Database references
Simbad data