STAR FORMATION IN 30 DORADUS

@article{Marchi2010STARFI,
  title={STAR FORMATION IN 30 DORADUS},
  author={Guido De Marchi and Francesco Paresce and Nino Panagia and Giacomo Beccari and Loredana Spezzi and Marco Sirianni and Morten Andersen and Max J. Mutchler and Bruce Balick and Michael A. Dopita and Jay. A. Frogel and Bradley C. Whitmore and Howard E. Bond and Daniela Clazetti and C. M. Carollo and Michael John Disney and Donald N. B. Hall and Jon A. Holtzman and Randy A. Kimble and Patrick McCarthy and Robert W. O’Connell and Abhijit Kumar Saha and Joseph I. Silk and John Terry Trauger and Alistair R. Walker and Rogier A. Windhorst and Erick T. Young},
  journal={The Astrophysical Journal},
  year={2010},
  volume={739},
  pages={27}
}
Using observations obtained with the Wide-Field Camera 3 on board the Hubble Space Telescope, we have studied the properties of the stellar populations in the central regions of 30 Dor in the Large Magellanic Cloud. The observations clearly reveal the presence of considerable differential extinction across the field. We characterize and quantify this effect using young massive main-sequence stars to derive a statistical reddening correction for most objects in the field. We then search for pre… 
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. V. Recent Star Formation in the 30 Dor Nebula
We report on the properties of the low-mass stars that recently formed in the central ~ 2.7'x2.7' of 30 Dor including the R136 cluster. Using the photometric catalogue of De Marchi et al. (2011c),
CLUES TO THE STAR FORMATION IN NGC 346 ACROSS TIME AND SPACE
We have studied the properties of the stellar populations in the field of the NGC 346 cluster in the Small Magellanic Cloud, using the results of a novel self-consistent method that provides a
Photometric determination of the mass accretion rates of pre-mainsequence stars – III. Results in the Large Magellanic Cloud
We present a multiwavelength study of three star-forming regions, spanning the age range 1–14 Myr, located between the 30 Doradus complex and supernova SN 1987A in the Large Magellanic Cloud (LMC).
A Double Cluster at the Core of 30 Doradus
Based on an analysis of data obtained with the Wide Field Camera 3 on the Hubble Space Telescope we report the identification of two distinct stellar populations in the core of the giant H II region
Photometric Determination of the Mass Accretion Rates of Pre-main-sequence Stars. IV. Recent Star Formation in NGC?602
We have studied the young stellar populations in NGC?602, in the Small Magellanic Cloud, using a novel method that we have developed to combine Hubble Space Telescope photometry in the V, I, and H?
Pre-main-sequence stars older than 8 Myr in the Eagle nebula
Attention is given to a population of 110 stars in the NGC 6611 cluster of the Eagle nebula that have prominent near-infrared excess and optical colours typical of pre-main-sequence (PMS) stars older
Probing interstellar extinction near the 30 Doradus nebula with red giant stars
We have studied the interstellar extinction in a field of 3' x 3' located about 6' SW of 30 Doradus in the Large Magellanic Cloud (LMC). Hubble Space Telescope observations in the U, B, V, I and
Star formation in the starburst cluster in NGC 3603
We have used new, deep, visible and near infrared observations of the compact starburst cluster in the giant HII region NGC 3603 and its surroundings with the WFC3 on HST and HAWK-I on the VLT to
The extinction law inside the 30 Doradus nebula
We have studied the interstellar extinction in a field of ~3' x 3' at the core of the 30 Doradus nebula, including the central R136 cluster, in the Large Magellanic Cloud. Observations at optical and
An HST Study of Star Formation in Star-Burst Clusters
Using the Hubble Space Telescope, we have undertaken a systematic study of pre main sequence (PMS) stars spanning a wide range of masses \((0.5-4 \, \mathrm{M}_{\odot })\), metallicities
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References

SHOWING 1-10 OF 56 REFERENCES
Stellar Populations in Three Outer Fields of the Large Magellanic Cloud
We present Hubble Space Telescope photometry for three fields in the outer disk of the Large Magellanic Cloud (LMC) extending approximately 4 mag below the faintest main-sequence turnoff. We cannot
PROGRESSIVE STAR FORMATION IN THE YOUNG GALACTIC SUPER STAR CLUSTER NGC 3603
Early Release Science observations of the cluster NGC 3603 with the WFC3 on the refurbished Hubble Space Telescope allow us to study its recent star formation history. Our analysis focuses on stars
Gas near the center of 30 Doradus as revealed by Hubble Space Telescope images
We present images of a 40 pc region of the 30 Doradus nebula centered about 1 arcminute north of the luminous star cluster R136 in the Large Magellanic Cloud. The region was imaged with the Hubble
Young Stellar Populations Around SN 1987A
We present the first results of a study of the stellar population in a region of 30 pc radius around SN 1987A, based on an analysis of multiband Hubble Space Telescope (HST) WFPC2 images. The
THE LOW-MASS INITIAL MASS FUNCTION IN THE 30 DORADUS STARBURST CLUSTER
We present deep Hubble Space Telescope NICMOS 2 F160W band observations of the central 56 '' x 57 '' (14 pc x 14.25 pc) region around R136 in the starburst cluster 30Dor (NGC 2070) located in the
The Low End of the Initial Mass Function in Young Large Magellanic Cloud Clusters. I. The Case of R136
We report the result of a study in which we have used very deep broadband V and I Wide Field Planetary Camera 2 images of the R136 cluster in the Large Magellanic Cloud from the Hubble Space
Star Formation in R136: A Cluster of O3 Stars Revealed by Hubble Space Telescope Spectroscopy*
The R136 cluster in 30 Doradus is the prototype super star cluster, and the only example sufficiently close that its massive star content can be studied directly. We have used the Hubble Space
Some Characteristics of Current Star Formation in the 30 Doradus Nebula Revealed by HST/NICMOS
The extensive "second generation" of star formation within the 30 Doradus Nebula, evidently triggered by the R136 central cluster around its periphery, has been imaged with the Near-Infrared Camera
PHOTOMETRIC DETERMINATION OF THE MASS ACCRETION RATES OF PRE-MAIN-SEQUENCE STARS. II. NGC 346 IN THE SMALL MAGELLANIC CLOUD*
We have studied the properties of the stellar populations in the field of the NGC 346 cluster in the Small Magellanic Cloud, using a novel self-consistent method that allows us to reliably identify
The Intermediate-Mass Population in the Core of the R136 Star Cluster*
R136, the compact, luminous star cluster at the center of the 30 Doradus nebula, represents an extreme mode of star formation. Yet it is unique among these kinds of objects in that it can be resolved
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