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  • Motte, F. (author)

Initial highlights of the HOBYS key program, the Herschel imaging survey of OB young stellar objects

  • Article/chapterEnglish2010

Publisher, publication year, extent ...

  • 2010-07-16
  • EDP Sciences,2010
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:su-51471
  • https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-51471URI
  • https://doi.org/10.1051/0004-6361/201014690DOI

Supplementary language notes

  • Language:English
  • Summary in:English

Part of subdatabase

Classification

  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • authorCount :49
  • We present the initial highlights of the HOBYS key program, which are based on Herschel images of the Rosette molecular complex and maps of the RCW120 H II region. Using both SPIRE at 250/350/500 mu m and PACS at 70/160 mu m or 100/160 mu m, the HOBYS survey provides an unbiased and complete census of intermediate-to high-mass young stellar objects, some of which are not detected by Spitzer. Key core properties, such as bolometric luminosity and mass (as derived from spectral energy distributions), are used to constrain their evolutionary stages. We identify a handful of high-mass prestellar cores and show that their lifetimes could be shorter in the Rosette molecular complex than in nearby low-mass star-forming regions. We also quantify the impact of expanding H II regions on the star formation process acting in both Rosette and RCW 120.

Subject headings and genre

Added entries (persons, corporate bodies, meetings, titles ...)

  • Zavagno, A. (author)
  • Bontemps, S. (author)
  • Schneider, N. (author)
  • Hennemann, M. (author)
  • Di Francesco, J. (author)
  • Andre, Ph. (author)
  • Saraceno, P. (author)
  • Griffin, M. (author)
  • Marston, A. (author)
  • Ward-Thompson, D. (author)
  • White, G. (author)
  • Minier, V. (author)
  • Men'shchikov, A. (author)
  • Hill, T. (author)
  • Abergel, A. (author)
  • Anderson, L. D. (author)
  • Aussel, H. (author)
  • Balog, Z. (author)
  • Baluteau, J. -P (author)
  • Bernard, J. -Ph. (author)
  • Cox, P. (author)
  • Csengeri, T. (author)
  • Deharveng, L. (author)
  • Didelon, P. (author)
  • di Giorgio, A. -M (author)
  • Hargrave, P. (author)
  • Huang, M. (author)
  • Kirk, J. (author)
  • Leeks, S. (author)
  • Li, J. Z. (author)
  • Martin, P. (author)
  • Molinari, S. (author)
  • Nguyen-Luong, Q. (author)
  • Olofsson, GöranStockholms universitet,Institutionen för astronomi(Swepub:su)olofsson (author)
  • Persi, P. (author)
  • Peretto, N. (author)
  • Pezzuto, S. (author)
  • Roussel, H. (author)
  • Russeil, D. (author)
  • Sadavoy, S. (author)
  • Sauvage, M. (author)
  • Sibthorpe, B. (author)
  • Spinoglio, L. (author)
  • Testi, L. (author)
  • Teyssier, D. (author)
  • Vavrek, R. (author)
  • Wilson, C. D. (author)
  • Woodcraft, A. (author)
  • Stockholms universitetInstitutionen för astronomi (creator_code:org_t)

Related titles

  • In:Astronomy and Astrophysics: EDP Sciences518, s. L77-0004-63611432-0746

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