scholarly journals Spectral Energy Distributions of M81 Globular Clusters in the BATC Multicolor Survey

2006 ◽  
Vol 118 (839) ◽  
pp. 98-106 ◽  
Author(s):  
Jun Ma ◽  
Xu Zhou ◽  
David Burstein ◽  
Jiansheng Chen ◽  
Zhaoji Jiang ◽  
...  
2006 ◽  
Vol 449 (1) ◽  
pp. 143-149 ◽  
Author(s):  
J. Ma ◽  
X. Zhou ◽  
D. Burstein ◽  
Y. Yang ◽  
Z. Fan ◽  
...  

2010 ◽  
Vol 139 (4) ◽  
pp. 1438-1450 ◽  
Author(s):  
Song Wang ◽  
Zhou Fan ◽  
Jun Ma ◽  
Richard de Grijs ◽  
Xu Zhou

2009 ◽  
Vol 137 (6) ◽  
pp. 4884-4896 ◽  
Author(s):  
Jun Ma ◽  
Zhou Fan ◽  
Richard de Grijs ◽  
Zhenyu Wu ◽  
Xu Zhou ◽  
...  

2003 ◽  
Vol 125 (2) ◽  
pp. 727-741 ◽  
Author(s):  
Linhua Jiang ◽  
Jun Ma ◽  
Xu Zhou ◽  
Jiansheng Chen ◽  
Hong Wu ◽  
...  

1993 ◽  
Vol 153 ◽  
pp. 343-344
Author(s):  
M.L. Malagnini ◽  
L.E. Pasinetti Fracassini ◽  
S. Covino ◽  
A. Buzzoni

A grid of synthetic spectral energy distributions, representative of old stellar populations, has been used to derive colors in different photometric systems, and to compare the theoretical predictions with observational data for galactic globular clusters.


2012 ◽  
Vol 8 (S295) ◽  
pp. 318-318
Author(s):  
Mireia Montes ◽  
José A. Acosta-Pulido ◽  
M. Almudena Prieto ◽  
Juan A. Fernández-Ontiveros

AbstractWe present a multiwavelength photometric analysis of the innermost (3×3 kpc2) Globular Clusters (GCs) of M87. Their Spectral Energy Distributions (SEDs) were built with J and Ks imaging obtained with NaCo at the VLT, along with HST UV-optical archival data. Using both Galatic GC templates and stellar population models, we derived ages (> 10 Gyr) and metallicities ([Fe/H]~ −0.7) for these clusters (e.g: Cohen et al. 1998). These GCs have lower metallicities than its host galaxy. This agrees with the idea that the GC population formed earlier than the bulk of the stars.


2020 ◽  
Vol 500 (3) ◽  
pp. 2859-2860
Author(s):  
A S G Robotham ◽  
S Bellstedt ◽  
C del P Lagos ◽  
J E Thorne ◽  
L J Davies ◽  
...  

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