GGCs database: globular cluster NGC 6341

Release 11.12 ("Hergest Ridge")

Selected: M 92

Parameters
Positional Parameters
cluster	NGC 6341
name	M 92
RA	17 17 07.39
Declination	+43 08 09.4
Galactic longitude	68.34
Galactic latitude	34.86
R sun	8.3
R gc	9.6
X	2.5
Y	6.3
Z	4.7
Photometric Parameters
E (B-V)	0.02
V HB	15.1
(m-M)	14.65
Vt	6.44
MVt	-8.21
(U-B)	0.01
(B-V)	0.63
(V-I)	0.88
S_RR	13.1
HBR	0.91
hbt	2
Structural Parameters
[Fe / H]	-2.31
SpT	F2
v_r	-120
err	0.1
v_LSR	-103.5
c	1.68
r_c	0.26
r_h	1.02
r_t	15.17
lg(tc)	7.96
lg(th)	9.02
mu_V	15.47
rho_v	4.3
Color-magnitude diagrams
author	Stetson, Peter B.; Harris, William E.
title	CCD photometry of the globular cluster M92
journal	Astronomical Journal, vol. 96, Sept. 1988, p. 909-975.
CM diagram

Description of NGC 6341
Messier 92 (also known as M92 or NGC 6341) is a globular cluster in the constellation Hercules. It was discovered by Johann Elert Bode in 1777 and independently rediscovered by Charles Messier on March 18, 1781. M92 is at a distance of about 26,000 light-years away from Earth. M92 is one of the brighter globular clusters in the northern hemisphere, but it is often overlooked by amateur astronomers because of its proximity to the even more spectacular Messier 13. Source: Wikipedia \| Notify inaccuracies
Image
Image of the cluster from the Digital Sky Survey
Other Resources for NGC 6341

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Selected biblio
Paper n. 1
VandenBerg, Don A.; Denissenkov, P. A.; Catelan, Marcio Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. I. M3, M15, and M92 2016, The Astrophysical Journal, Volume 827, Issue 1, 23 pp. (NGC 7078 NGC 5272 NGC 6341 )
Paper n. 2
Kamann, S.et al. The central dynamics of M3, M13, and M92: stringent limits on the masses of intermediate-mass black holes 2014, Astronomy & Astrophysics, Volume 566, A58, 24 pp. (NGC 5272 NGC 6218 NGC 6341 )
Paper n. 3
Di Cecco, A. et al. On the Density Profile of the Globular Cluster M92 2013, The Astronomical Journal, Volume 145, pag. 103 (NGC 6341 )
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Query processed at 09:29, 19th April
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