Herschel view of the large-scale structure in the Chamaeleon dark clouds

Article, Preprint English OPEN
Alves de Oliveira, C.; Schneider, N.; Merín, B.; Prusti, T.; Ribas, Á.; Cox, N. L. J.; Vavrek, R.; Könyves, V.; Arzoumanian, D.; Puga, E.; Pilbratt, G. L.; Kóspál, Á.; André, Ph.; Didelon, P.; Men’shchikov, A.; Royer, P.; Waelkens, C.; Bontemps, S.; Winston, E.; Spezzi, L.; (2014)
  • Journal: Astronomy and Astrophysics (issn: 0004-6361)
  • Related identifiers: doi: 10.1051/0004-6361/201423504
  • Subject: Astrophysics - Astrophysics of Galaxies
    arxiv: Astrophysics::Galaxy Astrophysics | Computer Science::Systems and Control | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Solar and Stellar Astrophysics

The Chamaeleon molecular cloud complex is one of the nearest star-forming sites encompassing three molecular clouds with a different star-formation history, from quiescent (Cha III) to actively forming stars (Cha II), and reaching the end of star-formation (Cha I). To c... View more
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