THE PHYSICAL STRUCTURE OF PROTOPLANETARY DISKS: THE SERPENS CLUSTER COMPARED WITH OTHER REGIONS

@article{Oliveira2013THEPS,
  title={THE PHYSICAL STRUCTURE OF PROTOPLANETARY DISKS: THE SERPENS CLUSTER COMPARED WITH OTHER REGIONS},
  author={I. Oliveira and B. Mer{\'i}n and K. Pontoppidan and E. Dishoeck},
  journal={The Astrophysical Journal},
  year={2013},
  volume={762},
  pages={128}
}
Spectral energy distributions are presented for 94 young stars surrounded by disks in the Serpens Molecular Cloud, based on photometry and Spitzer/IRS spectra. Most of the stars have spectroscopically determined spectral types. Taking a distance to the cloud of 415 pc rather than 259 pc, the distribution of ages is shifted to lower values, in the 1-3 Myr range, with a tail up to 10 Myr. The mass distribution spans 0.2-1.2 M ☉, with median mass of 0.7 M ☉. The distribution of fractional disk… Expand
NEW X-RAY-SELECTED PRE-MAIN-SEQUENCE MEMBERS OF THE SERPENS MOLECULAR CLOUD
Imaging the circumstellar environment of the young T Tauri star SU Aurigae

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