scholarly journals Disentangling the physical reality of star cluster candidates projected towards the inner disc of the Large Magellanic Cloud

2014 ◽  
Vol 440 (4) ◽  
pp. 3091-3099 ◽  
Author(s):  
Andrés E. Piatti
2012 ◽  
Vol 762 (1) ◽  
pp. 65 ◽  
Author(s):  
A. D. Mackey ◽  
G. S. Da Costa ◽  
A. M. N. Ferguson ◽  
D. Yong

2015 ◽  
Vol 149 (2) ◽  
pp. 52 ◽  
Author(s):  
Samyaday Choudhury ◽  
Annapurni Subramaniam ◽  
Andrés E. Piatti

1998 ◽  
Vol 499 (1) ◽  
pp. L53-L56 ◽  
Author(s):  
Rebecca A. W. Elson ◽  
Steinn Sigurdsson ◽  
Jarrod Hurley ◽  
Melvyn B. Davies ◽  
Gerard F. Gilmore

2012 ◽  
Vol 761 (1) ◽  
pp. L5 ◽  
Author(s):  
Stefan C. Keller ◽  
A. Dougal Mackey ◽  
Gary S. Da Costa

2011 ◽  
Vol 414 (3) ◽  
pp. 2204-2214 ◽  
Author(s):  
Stefano Rubele ◽  
Léo Girardi ◽  
Vera Kozhurina-Platais ◽  
Paul Goudfrooij ◽  
Leandro Kerber

2017 ◽  
Vol 470 (1) ◽  
pp. L77-L81 ◽  
Author(s):  
Andrés E. Piatti ◽  
Andrew Cole

Abstract We report that the serendipitous young Large Magellanic Cloud cluster NGC 1971 exhibits an extended main-sequence turn-off (eMSTO) possibly originated mostly by a real age spread. We used CT1 Washington photometry to produce a colour–magnitude diagram (CMD) with the fiducial cluster features. From its eMSTO, we estimated an age spread of ∼170 Myr (observed age range 100–280 Myr), once observational errors, stellar binarity, overall metallicity variations and stellar rotation effects were subtracted in quadrature from the observed age width.


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