Dust, Ice, and Gas In Time (DIGIT) Herschel program first results: a full PACS-SED scan of the gas line emission in protostar DK Chamaeleontis

Research output: Contribution to journalJournal articleResearchpeer-review

  • T. A. van Kempen
  • J. D. Green
  • N. J., II Evans
  • E. F. van Dishoeck
  • L. E. Kristensen
  • G. J. Herczeg
  • B. Merín
  • J. -E. Lee
  • Jildau Bouwman
  • B. Acke
  • M. Adamkovics
  • J. C. Augereau
  • E. Bergin
  • G. A. Blake
  • P. M. J. Brown
  • J. S. Carr
  • J. -H. Chen
  • L. Cieza
  • C. Dominik
  • C. P. Dullemond
  • M. M. Dunham
  • A. Glassgold
  • M. Guedel
  • P. M. Harvey
  • Th. Henning
  • M. R. Hogerheijde
  • D. Jaffe
  • H. J. Kim
  • Claudia Knez
  • J. H. Lacy
  • S. Maret
  • G. Meeus
  • R. Meijerink
  • G. D. Mulders
  • L. Mundy
  • J. Najita
  • J. Olofsson
  • K.M. Pontoppidan
  • Colette Salyk
  • B. Sturm
  • R. Visser
  • L. B. F. M. Waters
  • C. Waelkens
  • U. A. Yildiz
Original languageEnglish
Article numberL128
JournalAstronomy & Astrophysics
Volume518
Number of pages5
ISSN0004-6361
DOIs
Publication statusPublished - 2010

    Research areas

  • astrochemistry, circumstellar matter, stars: formation, stars: protostars, infrared: ISM, submillimeter: ISM

ID: 176345017