Release 7.11 ("Paola")

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Your query: M 19

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Parameters
Positional Parameters
clusterNGC 6273
nameM 19
RA17 02 37.
Declination-26 16 05
Galactic longitude356.87
Galactic latitude9.38
R sun8.6
R gc1.6
X8.5
Y-0.5
Z1.4
Photometric Parameters
E (B-V)0.41
V HB16.5
(m-M)15.95
Vt6.77
MVt-9.08
(U-B)0.35
(B-V)1.03
(V-R)0.66
(V-I)1.35
S_RR0.2
hbt0
Structural Parameters
[Fe / H]-1.68
SpT F7
v_r135
err4
v_LSR145.6
c1.53
r_c0.43
r_h1.25
r_t14.5
lg(tc)8.5
lg(th)9.35
mu_V16.82
rho_v3.96
Color-magnitude diagrams
authorPiotto, G.; Zoccali, M.; King, I. R.; Djorgovski, S. G.; Sosin, C.; Rich, R. M.; Meylan, G.
titleHUBBLE SPACE TELESCOPE Observations of Galactic Globular Cluster Cores. II. NGC 6273 and the Problem of Horizontal-Branch Gaps
journalThe Astronomical Journal, Volume 118, Issue 4, pp. 1727-1737 (1999)
CM diagram
CreditsCMD from Padova database
Description of NGC 6273

Messier 19 (also known as M19 or NGC 6273) is a globular cluster in the constellation Ophiuchus. It was discovered by Charles Messier in 1764 and added to his catalog of comet-like objects that same year.

M19 is the most oblate known globular cluster. It is at a distance of about 28,000 light-years from the Solar System, and quite near to the Galactic Center, only about 5,200 light-years away.

Source: Wikipedia | Notify inaccuracies

DSS image

Image of the cluster from the Digital Sky Survey

Other Resources
for NGC 6273
ADS "Object Search"
SEDS data
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Selected biblio
Paper n. 1
Piotto, G.; Zoccali, M.; King, I. R.; Djorgovski, S. G.; Sosin, C.; Rich, R. M.; Meylan, G.
HUBBLE SPACE TELESCOPE Observations of Galactic Globular Cluster Cores. II. NGC 6273 and the Problem of Horizontal-Branch Gaps
The Astronomical Journal, Volume 118, Issue 4, pp. 1727-1737 (1999)
(NGC 6273 cmd )
See all items (1 paper)

Query processed at 21:27, 9th February
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