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

By Fr'ed'erique Motte, A. Zavagno, S. Bontemps, Nathan Schneider, M. Hennemann, J. Francesco, P. Andre', P. Saraceno, M. Gri, A. Marston and 39 more. 2010

144 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Spectroscopy

View Paper: https://www.semanticscholar.org/paper/866b6cfb5eca506e87ee838b823b51ba5ddad018

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Citations in the corpus

The spine of the swan: a Herschel study of the DR21 ridge and filaments in Cygnus X (2012, methodology): “The Herschel imaging survey of OB Young Stellar objects (HOBYS, Motte et al. 2010) observes massive molecular cloud complexes within 3 kpc distance to probe the cloud environment of OB star-forming cores, their statistical evolu- ?”
Planckearly results. XXV. Thermal dust in nearby molecular clouds (2011, background): “…& Bally 1999), by balloon-borne experiments PRONAOS (Ristorcelli et al. 1998), Archeops (Désert et al. 2008) and BLAST (Netterﬁeld et al. 2009), and from space by Spitzer (e.g., Flagey et al. 2009) and Herschel (e.g., André et al. 2010; Motte et al. 2010; Abergel et al. 2010; Juvela et al. 2011).”
A multi-scale, multi-wavelength source extraction method: getsources (2012, methodology): “Furthermore, the Herschel HOBYS survey (Motte et al. 2010) aims at performing a census of massive young stellar objects, providing accurate bolometric luminosities and envelope masses for homogeneous and complete samples of the progenitors of massive stars.”
The ATLASGAL survey: a catalog of dust condensations in the Galactic plane (2013, methodology): “Therefore several new methods have been developed to deal with the extended emission and also to handle multiwavelength data sets such as those of Herschel (e.g.MRE-GCL, Multi-resolution and Gaussclumps algorithm,Motte et al. 2010, CuTeX: Molinari et al. 2011,Getsources:Men’shchikov et al. 2012).”
A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey (2015, background): “…Men’shchikov et al. 2010; Miville-Deschênes et al. 2010) and other imaging surveys such as HiGAL (Molinari et al. 2010; Schisano et al. 2014), HOBYS (Motte et al. 2010; Hill et al. 2011), and EPoS (Henning et al. 2010) now demonstrate that these filaments are truly ubiquitous in the cold ISM,…”
Cluster-formation in the Rosette molecular cloud at the junctions of filaments (2012, unknown): “Existing infrared (IR) clusters and the most massive dense cores (MDCs) identified in the same data set (Motte et al. 2010; Hennemann et al. 2010) are overlaid on the image.”
WHAT DETERMINES THE DENSITY STRUCTURE OF MOLECULAR CLOUDS? A CASE STUDY OF ORION B WITH HERSCHEL (2013, background): “The spatial structure of clouds, now impressively revealed by Herschel imaging observations in the far-infrared (e.g., André et al. (2010), Motte et al. (2010), Molinari et al. (2010)), is very inhomogeneous and dominated by filaments (Arzoumanian et al. (2011), Schneider et al. (2012)).”
Filaments and ridges in Vela C revealed by Herschel: from low-mass to high-mass star-forming sites (2011, methodology): “Sources were identified using the multi-wavelength multi-resolution getsources extraction routine (Men’shchikov et al. 2010) which is consistent with the MRE-GCL algorithm (Motte et al. 2003) used for the HOBYS programme during the Herschel science demonstration phase (e.g. Motte et al. 2010).”
Planck 2015 results - XXVIII. The Planck Catalogue of Galactic cold clumps (2015, unknown): “…of the sky covered by other Herschel Key Programmes, such as the Galactic plane for | b | < 1 ◦ , which was targeted by the Hi-GAL programme (Molinari et al. 2010), and several nearby clouds that are included in the Gould Belt (André et al. 2010) and HOBYS (e.g., Motte et al. 2010) programmes.”