SUPER STAR CLUSTERS IN SBS0335-052E

Thompson, RI; Sauvage M.; Kennicutt, RC; Engelbracht, C.; Vanzi L.; Schneider G.

Abstract

As one of the lowest metallicity star-forming galaxies, with a nucleus of several super star clusters (SSCs), SBS0335-052E is the subject of substantial current study. We present new insights on this galaxy based on new and archival high spatial resolution NICMOS and attitude control system images. We provide new measurements and limits on the size of several of the SSCs. The images have sufficient resolution to divide the star formation into compact regions and newly discovered extended regions, indicating a bimodal form of star formation. The star formation regions are dated via the equivalent width of the Paa emission and we find that two of the extended regions of star formation are less than 10 million years old. Our previous finding that stellar winds confine the photo-ionizing flux to small regions around individual stars is consistent with the new observations. This may allow planet formation in what would traditionally be considered a harsh environment and has implications for the number of planets around globular cluster stars. In addition, the images pinpoint the regions of H2 emission as located in, but not at the center of, the two star-forming super star clusters, S1 and S2. © 2009. The American Astronomical Society. All rights reserved..

Más información

Título según WOS: SUPER STAR CLUSTERS IN SBS0335-052E
Título según SCOPUS: Super star clusters in SBS0335-052E
Título de la Revista: ASTROPHYSICAL JOURNAL
Volumen: 691
Número: 2
Editorial: IOP PUBLISHING LTD
Fecha de publicación: 2009
Página de inicio: 1068
Página final: 1078
Idioma: English
URL: http://stacks.iop.org/0004-637X/691/i=2/a=1068?key=crossref.de898f0ff8e0f884d867e26e7a8f0cd1
DOI:

10.1088/0004-637X/691/2/1068

Notas: ISI, SCOPUS