Release 7.11 ("Paola")

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Your query: M 71

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Parameters
Positional Parameters
clusterNGC 6838
nameM 71
RA19 53 46.
Declination+18 46 42
Galactic longitude56.74
Galactic latitude-4.56
R sun4
R gc6.7
X2.2
Y3.3
Z-0.3
Photometric Parameters
E (B-V)0.25
V HB14.48
(m-M)13.79
Vt8.19
MVt-5.56
(U-B)0.63
(B-V)1.09
(V-R)0.63
(V-I)1.36
S_RR0
HBR-1
hbt7
Structural Parameters
[Fe / H]-0.73
SpT G1
v_r-22.8
err0.2
v_LSR-5.5
c1.15
r_c0.63
r_h1.65
r_t8.96
lg(tc)7.64
lg(th)8.43
mu_V19.22
rho_v3.05
Color-magnitude diagrams
authorHodder, Philip J. C.; Nemec, James M.; Richer, Harvey B.; Fahlman, Gregory G.
titleDeep CCD photometry and variable stars in the metal-rich globular cluster M71
journalAstronomical Journal, vol. 103, Feb. 1992, p. 460
CM diagram
Description of NGC 6838

Messier 71 (also known as M71 or NGC 6838) is a globular cluster in the constellation Sagitta. It was discovered by Philippe Loys de Cheseaux in 1746 and included by Charles Messier in his catalog of comet-like objects in 1780. It was also noted by Koehler at Dresden around 1775.

M71 is at a distance of about 12,000 light years away from Earth and spans some 27 light years across. The irregular variable star Z Sagittae is a member of this cluster.

M71 was long thought (until the 1970s) to be a densely packed open cluster and was classified as such by leading astronomers in the field of star cluster research due to its lacking a dense central compression (..) However, modern photometric photometry has detected a short "horizontal branch" in the H-R diagram of M71, which is characteristic of a globular cluster.

Source: Wikipedia | Notify inaccuracies

DSS image

Image of the cluster from the Digital Sky Survey

Other Resources
for NGC 6838
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Selected biblio
Paper n. 1
Hodder, Philip J. C.; Nemec, James M.; Richer, Harvey B.; Fahlman, Gregory G.
Deep CCD photometry and variable stars in the metal-rich globular cluster M71
Astronomical Journal, vol. 103, Feb. 1992, p. 460
(NGC 6838 cmd )
See all items (1 paper)

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