Probing the anomalous extinction of four young star clusters: the use of colour-excess, main-sequence fitting and fractal analysis


Autoria(s): Fernandes, B.; Gregorio-Hetem, J.; Hetem, A., Jr.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

01/11/2013

01/11/2013

2012

Resumo

Aims. We studied four young star clusters to characterise their anomalous extinction or variable reddening and asses whether they could be due to contamination by either dense clouds or circumstellar effects. Methods. We evaluated the extinction law (R-V) by adopting two methods: (i) the use of theoretical expressions based on the colour-excess of stars with known spectral type; and (ii) the analysis of two-colour diagrams, where the slope of the observed colour distribution was compared to the normal distribution. An algorithm to reproduce the zero-age main-sequence (ZAMS) reddened colours was developed to derive the average visual extinction (A(V)) that provides the closest fit to the observational data. The structure of the clouds was evaluated by means of a statistical fractal analysis, designed to compare their geometric structure with the spatial distribution of the cluster members. Results. The cluster NGC 6530 is the only object of our sample affected by anomalous extinction. On average, the other clusters suffer normal extinction, but several of their members, mainly in NGC 2264, seem to have high R-V, probably because of circumstellar effects. The ZAMS fitting provides A(V) values that are in good agreement with those found in the literature. The fractal analysis shows that NGC 6530 has a centrally concentrated distribution of stars that differs from the substructures found in the density distribution of the cloud projected in the A(V) map, suggesting that the original cloud was changed by the cluster formation. However, the fractal dimension and statistical parameters of Berkeley 86, NGC 2244, and NGC 2264 indicate that there is a good cloud-cluster correlation, when compared to other works based on an artificial distribution of points.

CAPESCOFECUB

CAPES/Cofecub [712/2011]

CNPq

CNPq [142849/2010-3]

National Aeronautics and Space Administration

National Aeronautics and Space Administration

National Science Foundation

National Science Foundation

Identificador

ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, v. 541, n. 2, supl. 1, Part 2, pp. 707-712, MAY, 2012

0004-6361

http://www.producao.usp.br/handle/BDPI/37137

10.1051/0004-6361/201117677

http://dx.doi.org/10.1051/0004-6361/201117677

Idioma(s)

eng

Publicador

EDP SCIENCES S A

LES ULIS CEDEX A

Relação

ASTRONOMY & ASTROPHYSICS

Direitos

restrictedAccess

Copyright EDP SCIENCES S A

Palavras-Chave #DUST, EXTINCTION #STARS: PRE-MAIN SEQUENCE #METHODS: STATISTICAL #H-ALPHA PHOTOMETRY #MOLECULAR CLOUDS #NGC 6530 #SPECTRAL CLASSIFICATION #INTERSTELLAR EXTINCTION #NONUNIFORM EXTINCTION #ABNORMAL EXTINCTION #EMBEDDED CLUSTERS #STELLAR CONTENTS #NGC-2244 #ASTRONOMY & ASTROPHYSICS
Tipo

article

original article

publishedVersion