scholarly journals Near-Infrared Photometry of the Globular Cluster Palomar 6

2002 ◽  
Vol 123 (6) ◽  
pp. 3305-3317 ◽  
Author(s):  
Jae-Woo Lee ◽  
Bruce W. Carney
2014 ◽  
Vol 446 (1) ◽  
pp. 730-736 ◽  
Author(s):  
A. T. Valcheva ◽  
E. P. Ovcharov ◽  
A. D. Lalova ◽  
P. L. Nedialkov ◽  
V. D. Ivanov ◽  
...  

2007 ◽  
Vol 476 (1) ◽  
pp. 243-253 ◽  
Author(s):  
M. Salaris ◽  
E. V. Held ◽  
S. Ortolani ◽  
M. Gullieuszik ◽  
Y. Momany

Author(s):  
M. Dall'Ora ◽  
J. Storm ◽  
G. Bono ◽  
P. B. Stetson ◽  
G. Andreuzzi ◽  
...  

2002 ◽  
Vol 207 ◽  
pp. 107-109 ◽  
Author(s):  
J. Borissova ◽  
V. D. Ivanov ◽  
L. Vanzi

We present a preliminary report on the first deep near infrared photometry of 2MASS GC 01 and 2MASS GC 02 - new Galactic globular cluster candidates, discovered by the 2MASS. The red giant branch slopes yielded [Fe/H]=-0.42 ± 0.15 dex and [Fe/H]=-0.66 ± 0.17 dex, respectively for GC 01 and GC 02. We estimated the reddening towards GC 01 and GC 02: E(B - V) = 5.36 ± 0.20, and E(B - V) = 4.55 ± 0.17. The calculated distance moduli to the clusters are: (m - M)0 = 13.53 ± 0.27 and (m - M)0 = 14.53 ± 0.31 for GC 01 and GC 02. Our best fit for the radial surface brightness profile of GC 02 yields: lg(rc) = 1.40, lg(rh) = 1.54, lg(rt) = 1.31, and c=1.60. CC 01 is less concentrated: lg(rc) = 1.63, lg(rh) = 1.7, lg(rt) = 1.25, and c=1.41.


2016 ◽  
Vol 462 (1) ◽  
pp. 501-510 ◽  
Author(s):  
Julio A. Carballo-Bello ◽  
S. Ramírez Alegría ◽  
J. Borissova ◽  
L. C. Smith ◽  
R. Kurtev ◽  
...  

1986 ◽  
Vol 10 (1) ◽  
pp. 62-66 ◽  
Author(s):  
Ke-ping Zhou ◽  
Yun-xiang Hao ◽  
Pei-sheng Chen ◽  
Yun Zhang ◽  
Heng Gao

2003 ◽  
Vol 55 (1) ◽  
pp. 103-119 ◽  
Author(s):  
Kotaro Kohno ◽  
Baltasar Vila-Vilaró ◽  
Seiichi Sakamoto ◽  
Ryohei Kawabe ◽  
Sumio Ishizuki ◽  
...  

2001 ◽  
Vol 122 (6) ◽  
pp. 3136-3154 ◽  
Author(s):  
Jae-Woo Lee ◽  
Bruce W. Carney ◽  
Laura K. Fullton ◽  
Peter B. Stetson

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