Release 11.12 ("Hergest Ridge")


Selected: NGC 4147

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Parameters
Positional Parameters
clusterNGC 4147
RA12 10 06.30
Declination+18 32 33.5
Galactic longitude252.85
Galactic latitude77.19
R sun19.3
R gc21.4
X-1.3
Y-4.1
Z18.8
Photometric Parameters
E (B-V)0.02
V HB17.02
(m-M)16.49
Vt10.32
MVt-6.17
(U-B)0.11
(B-V)0.59
(V-R)0.42
(V-I)0.79
S_RR30.8
HBR0.55
hbt3
Structural Parameters
[Fe / H]-1.8
SpTF2/3
v_r183.2
err0.7
v_LSR186.1
c1.83
r_c0.09
r_h0.48
r_t6.31
lg(tc)7.41
lg(th)8.74
mu_V17.38
rho_v3.63
Color-magnitude diagrams
authorWang, J. J.; Chen, L.; Wu, Z. Y.; Gupta, A. C.; Geffert, M.
titleKinematics and CMD of the globular cluster NGC 4147
journalAstronomy and Astrophysics Supplement, v.142, p.373-387
CM diagram
Description of NGC 4147

Globular cluster NGC 4147 was discovered by William Herschel on March 14, 1784 and cataloged as H I.19.

This cluster is perhaps a former member of the Sagittarius Dwarf Elliptical Galaxy (SagDEG), or Sagittarius Dwarf Spheroidal Galaxy (Sgr dSph), the nearby dwarf galaxy discovered in 1994, which is currently in a close and perhaps final encounter before its tidal disruption, with our Milky Way Galaxy.

Source: SEDS | Notify inaccuracies

Image

Image of the cluster from the Digital Sky Survey

Other Resources
for NGC 4147
ADS "Object Search"
C. Clement variables data
SEDS data
Google Sky
Web Links for this cluster
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Users comments for this cluster
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Selected biblio
Paper n. 1
Stetson, Peter B.; Catelan, M.; Smith, Horace A.
Homogeneous Photometry. V. The Globular Cluster NGC 4147
2005, PASP, Vol. 117, Pagg. 1325-1361
(NGC 4147 )
Paper n. 2
Wang, J. J.; Chen, L.; Wu, Z. Y.; Gupta, A. C.; Geffert, M.
Kinematics and CMD of the globular cluster NGC 4147
2000, Astronomy and Astrophysics Supplement, v.142, p.373-387
(NGC 4147 )
Paper n. 3
Auriere, M.; Lauzeral, C.
CCD photometry in the central region of the globular cluster NGC 4147
1991, stronomy and Astrophysics, vol. 244, no. 2, April 1991, p. 303-309
(NGC 4147 cmd )
See all items (3 papers) :: Submit a paper
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Query processed at 03:21, 18th April
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