Hubble Space Telescope Photometry of Hodge 301: An "Old" Star Cluster in 30 Doradus

Details Hubble Space Telescope Photometry of Hodge 301: An "Old" Star Cluster in 30 Doradus Hubble Space Telescope Photometry of Hodge 301: An "Old" Star Cluster in 30 Doradus

1999-10-22

arxiv.org/abs/astro-ph/9910426v1

2000, AJ, 119, 787-799

Astronomy and Astrophysics

Astrophysics

To appear in the Astronomical Journal (Feb 2000 issue). 16 pages in two-column style. 9 separate figures, in part in significa

Scientific paper

10.1086/301218

We present Hubble Space Telescope Planetary Camera UVI data for the little-studied cluster Hodge 301 3' northwest of 30 Doradus' central ionizing cluster R136. The average reddening of Hodge 301 is found to be = (0.28+-0.05) mag from published infrared and ultraviolet photometry. Using two different sets of evolutionary models, we derive an age of ~ 20-25 Myr for Hodge 301, which makes it roughly 10 times as old as R136. Hodge 301 is the most prominent representative of the oldest population in the 30 Dor starburst region; a region that has undergone multiple star formation events. This range of ages is an important consideration for the modelling of starburst regions. Hodge 301 shows a widened upper main sequence largely caused by Be stars. We present a list of Be star candidates. The slope of the initial mass function for intermediate-mass main sequence stars ranging from 10 to 1.3 solar masses is found to be -1.4+-0.1 in good agreement with a Salpeter law. There is no indication for a truncation or change of slope of the IMF within this mass range. In accordance with the age of Hodge 301 no obvious pre-main-sequence stars are seen down to 1 solar mass. We estimate that up to 41+-7 stars with more than 12 solar masses may have turned into supernovae since the formation of the cluster. Multiple supernova explosions are the most likely origin of the extremely violent gas motions and the diffuse X-ray emission observed in the cluster surroundings.

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