Release 7.11 ("Paola")

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Your query: M 28

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Parameters
Positional Parameters
clusterNGC 6626
nameM 28
RA18 24 32.
Declination-24 52 12
Galactic longitude7.8
Galactic latitude-5.58
R sun5.6
R gc2.7
X5.5
Y0.8
Z-0.5
Photometric Parameters
E (B-V)0.4
V HB15.55
(m-M)14.97
Vt6.79
MVt-8.33
(U-B)0.46
(B-V)1.08
(V-R)0.69
(V-I)1.41
S_RR5.4
HBR0.9
hbt2
Structural Parameters
[Fe / H]-1.45
SpT F8
v_r17
err1
v_LSR28.5
c1.67
r_c0.24
r_h1.56
r_t11.27
lg(tc)7.62
lg(th)9.04
mu_V16.08
rho_v4.75
Color-magnitude diagrams
authorTesta, Vincenzo; Corsi, Carlo E.; Andreuzzi, Gloria; Iannicola, Giacinto;
Marconi, Gianni; Piersimoni, Anna Marina; Buonanno Roberto
titleHorizontal-Branch Morphology and Dense Environments:
Hubble Space Telescope Observations of Globular Clusters NGC 2298, 5897, 6535, and 6626
journalThe Astronomical Journal, Volume 121, Issue 2, pp. 916-934 (2001)
CM diagram
Description of NGC 6626

Messier 28 (also known as M28 or NGC 6626) is a globular cluster in the constellation Sagittarius. It was discovered by Charles Messier in 1764.

M28 is at a distance of about 18,000 to 19,000 light-years away from Earth. 18 RR Lyrae type variable stars have been observed in this cluster. In 1986, M28 became the first globular cluster where a millisecond pulsar was discovered (by the Lovell Telescope at Jodrell Bank Observatory).

Source: Wikipedia | Notify inaccuracies

DSS image

Image of the cluster from the Digital Sky Survey

Other Resources
for NGC 6626
ADS "Object Search"
SEDS data
Web Links for this cluster
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Users comments for this cluster
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Selected biblio
Paper n. 1
Testa, Vincenzo; Corsi, Carlo E.; Andreuzzi, Gloria; Iannicola, Giacinto;
Marconi, Gianni; Piersimoni, Anna Marina; Buonanno Roberto

Horizontal-Branch Morphology and Dense Environments:
Hubble Space Telescope Observations of Globular Clusters NGC 2298, 5897, 6535, and 6626

The Astronomical Journal, Volume 121, Issue 2, pp. 916-934 (2001)
(NGC 6626 cmd )
See all items (1 paper)

Query processed at 21:41, 9th February
This page has been visited 4541 times, since Oct 25 2004


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