NGC 5490

NGC 5490
	NGC 5490 , Radio Galaxy.
Observation data (J2000 epoch)
Constellation	Boötes
Right ascension	14h 09m 57.330s[1]
Declination	+17° 32′ 43.53″[1]
Redshift	0.016693[2]; (5,008 km/s)
Distance	225.63 ± 0.29 Mly (69.18 ± 0.09 Mpc)[3]
Apparent magnitude (V)	12.9[4]
Characteristics
Type	E[4]
Apparent size (V)	1.443′ × 1.126′[1]
Notable features	See also Gra 1408+17
Other designations
	2MASX J14095733+1732435, 4C 17.57, CGCG 103.095, GC 3798, H III-32, h 1752, LEDA 50558, LGG 376-001, MITG J1409+1732, MCG+03-36-065, MRC 1407+177, OHIO Q 112, PGC 50558, PKS 1407+17, UGC 9058, UT 1407+178, UZC J140957.3+173244, VRO 17.14.01, Z 103-95, Z 1407.6+1747

NGC 5490 is a radio galaxy in the constellation Boötes.

Gra 1408+17

Gra 1408+17 is a radio-source in NGC 5490, located at the coordinates: RA 14^h 10.4^m, Dec. +17° 32′; Galactic coordinates J2000 : 009.27 ± 180000, +69.41 ± 180000.

gollark: It doesn't even bother to add newlines!

gollark: ```pythonclass Entry(ℝ): def __init__(self, Matrix=globals()): M_ = collections.defaultdict(__import__("functools").lru_cache((lambda _: lambda: -0)(lambda: lambda: 0))) M_[0] = [*map(lambda dabmal: random.randint(0, len(Row)), range(10))] for self in repr(aes256): for i in range(ℤ(math.gamma(0.5)), ℤ(math.gamma(7))): print(" #"[i in M_[0]], end="") M_[1] = {*lookup[10:]} for M_[3] in [ marshal for t in [*(y for y in (x for x in map(lambda p: range(p - 1, p + 2), M_[0])))] for marshal in t ]: M_[4] = (((M_[3] - 1) in M_[0]) << 2) + ((M_[3] in M_[0]) << 1) + ((M_[3] + 1) in M_[0]) if (0o156&(1<<M_[4]))>>M_[4]: M_[1].add(M_[3]) M_[0] = M_[1] pass passpass```Sheer elegance.

gollark: Apparently nobody noticed the random rule 110 implementation *either*.

gollark: Although I guess mine could and probably did as I never revealed what the obfuscated code did.

gollark: Hmm. I really wonder *what* palaiologos's code does. It could probably have uploaded secret bee neuron data to palaiologos' server and nobody would know.

References

Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.
Kochanek, C. S.; et al. (October 2001), "The K-Band Galaxy Luminosity Function", The Astrophysical Journal, 560 (2): 566–579, arXiv:astro-ph/0011456, Bibcode:2001ApJ...560..566K, doi:10.1086/322488.
Tully, R. Brent; et al. (October 2013), "Cosmicflows-2: The Data", The Astronomical Journal, 146 (4): 25, arXiv:1307.7213, Bibcode:2013AJ....146...86T, doi:10.1088/0004-6256/146/4/86, 86.
"NED results for object NGC 5490", NASA/IPAC Extragalactic Database, retrieved 2015-10-29.

External links

Database references
Simbad	data

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.

[ApJ131_1163-1] Skrutskie, M. F.; et al. (February 2006), "The Two Micron All Sky Survey (2MASS)", The Astronomical Journal, 131 (2): 1163–1183, Bibcode:2006AJ....131.1163S, doi:10.1086/498708.

[apj560_2_566-2] Kochanek, C. S.; et al. (October 2001), "The K-Band Galaxy Luminosity Function", The Astrophysical Journal, 560 (2): 566–579, arXiv:astro-ph/0011456, Bibcode:2001ApJ...560..566K, doi:10.1086/322488.

[aj146_86-3] Tully, R. Brent; et al. (October 2013), "Cosmicflows-2: The Data", The Astronomical Journal, 146 (4): 25, arXiv:1307.7213, Bibcode:2013AJ....146...86T, doi:10.1088/0004-6256/146/4/86, 86.

[ned-4] "NED results for object NGC 5490", NASA/IPAC Extragalactic Database, retrieved 2015-10-29.