Spectra of the two brightest objects in the amorphous galaxy NGC 1569 - Superluminous young star clusters-or stars in a nearby peculiar galaxy?

1985 ◽  
Vol 90 ◽  
pp. 1163 ◽  
Author(s):  
H. Arp ◽  
A. Sandage
2010 ◽  
Vol 43 (1) ◽  
pp. 1-8 ◽  
Author(s):  
Jae-Mann Kyeong ◽  
Eon-Chang Sung ◽  
Sang-Chul Kim ◽  
Brian Chaboyer

2008 ◽  
Vol 385 (2) ◽  
pp. 929-938 ◽  
Author(s):  
Vasilii V. Gvaramadze ◽  
Alessia Gualandris ◽  
Simon Portegies Zwart

2008 ◽  
Vol 489 (3) ◽  
pp. 1091-1105 ◽  
Author(s):  
S. Mengel ◽  
M. D. Lehnert ◽  
N. A. Thatte ◽  
W. D. Vacca ◽  
B. Whitmore ◽  
...  

2008 ◽  
Vol 389 (1) ◽  
pp. 429-440 ◽  
Author(s):  
Andrés E. Piatti ◽  
Doug Geisler ◽  
Ata Sarajedini ◽  
Carme Gallart ◽  
Marina Wischnjewsky

2003 ◽  
Vol 598 (2) ◽  
pp. 1000-1004 ◽  
Author(s):  
Letizia Stanghellini ◽  
Eva Villaver ◽  
Richard A. Shaw ◽  
Max Mutchler

2003 ◽  
Vol 585 (2) ◽  
pp. 750-755 ◽  
Author(s):  
H. D. Tran ◽  
M. Sirianni ◽  
H. C. Ford ◽  
G. D. Illingworth ◽  
M. Clampin ◽  
...  

1991 ◽  
Vol 148 ◽  
pp. 207-208
Author(s):  
Myung Gyoon Lee

Using U BV CCD photometry, the stellar content of HII regions and young star clusters in the Magellanic Clouds has been studied: (1) the reddenings have been determined, and ages of OB associations and young star clusters have been measured; (2) the stellar initial mass functions have been determined by using the main-sequence luminosity functions; and (3) U BV CCD surface photometry of nine young star clusters has been obtained and their structural properties investigated.


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