2001/04/17 by Wolfgang Brandner, W. Brandner, E. K. Grebel +7 · 2 citations
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Initial mass function #Large Magellanic Cloud #Physics #Population #Protostar #Star cluster #Star formation #Stars #Stellar population #Stellar, planetary, and galactic studies #T Tauri star #astro-ph
paper · pdf · doi:10.1086/322065
published as Astron.J.122:858-865,2001 · 9 pages, 4 figures, uses emulateapj.sty and psfig.sty. accepted for publication in the Astronomical Journal (August 2001 issue)
arxiv created 2001/04/17 · openalex publication_date 2001/08/01 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present the detection of an intermediate-mass, pre–main-sequence population embedded in the nebular filaments surrounding the 30 Doradus region in the Large Magellanic Cloud (LMC) using HST /NICMOS. In addition to four previously known luminous Class I infrared "protostars," the NICMOS data reveal 20 new sources with intrinsic infrared excess similar to Galactic pre–main-sequence stars. Based on their infrared brightness, these objects can be identified as the LMC equivalent of Galactic pre–main-sequence stars. The faintest LMC young stellar objects in the sample have colors similar to T Tauri stars and have about the same brightness as T Tauri stars if placed at the distance of the LMC. We find no evidence for a lower mass cutoff in the initial mass function. Instead, the whole spectrum of stellar masses from pre–main-sequence stars with ∼1.5 M ⊙ to massive O stars still embedded in dense knots appears to be present in the nebular filaments. The majority of the young stellar objects can be found to the north of the central starburst cluster R136. This region is very likely evolving into an OB association. The observations provide further evidence that star formation in the 30 Doradus region is very similar to Galactic star formation and confirm the presence of sequential star formation in 30 Doradus, with present-day star formation taking place in the arc of molecular gas to the north and west of the starburst cluster.