B. Horeau
Paris Diderot University
2 Papers
2 Citations
B. Horeau is an academic researcher from Paris Diderot University. The author has contributed to research in topics: Luminosity & Star formation. The author has an hindex of 1, co-authored 2 publications.
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Papers
Herschel observations of embedded protostellar clusters in the Rosette Molecular Cloud
Martin Hennemann,Frédérique Motte,Sylvain Bontemps,Sylvain Bontemps,Nicola Schneider,T. Csengeri,Zoltan Balog,J. Di Francesco,Annie Zavagno,Ph. André,Alexander Men'shchikov,Alain Abergel,Babar Ali,J.-P. Baluteau,J.-Ph. Bernard,Pierre Cox,P. Didelon,A. Di Giorgio,Matthew Joseph Griffin,Peter Charles Hargrave,T. Hill,B. Horeau,Maohai Huang,Jason M. Kirk,S. J. Leeks,Jin-Zeng Li,A. Marston,Peter G. Martin,Sergio Molinari,Q. Nguyen Luong,Göran Olofsson,Paolo Persi,Stefano Pezzuto,D. Russeil,P. Saraceno,Marc Sauvage,Bruce Sibthorpe,L. Spinoglio,Leonardo Testi,Derek Ward-Thompson,Glenn J. White,Glenn J. White,C. D. Wilson,Adam Woodcraft +43 more
TL;DR: In this paper, a sample of protostars and their spectral energy distributions that covers the near-infrared to sub-millimetre wavelength range were used to constrain key properties in the protostellar evolution, bolometric luminosity, and envelope mass.
Herschel observations of embedded protostellar clusters in the Rosette Molecular Cloud
Martin Hennemann,Frédérique Motte,Sylvain Bontemps,Sylvain Bontemps,Nicola Schneider,T. Csengeri,Zoltan Balog,J. Di Francesco,Annie Zavagno,Ph. André,Alexander Men'shchikov,Alain Abergel,Babar Ali,J.-P. Baluteau,J.-Ph. Bernard,Pierre Cox,P. Didelon,A. Di Giorgio,Matthew Joseph Griffin,Peter Charles Hargrave,T. Hill,B. Horeau,Maohai Huang,Jason M. Kirk,S. J. Leeks,Jin-Zeng Li,A. Marston,Peter G. Martin,Sergio Molinari,Q. Nguyen Luong,Göran Olofsson,Paolo Persi,Stefano Pezzuto,D. Russeil,P. Saraceno,Marc Sauvage,Bruce Sibthorpe,L. Spinoglio,Leonardo Testi,Derek Ward-Thompson,Glenn J. White,Glenn J. White,C. D. Wilson,Adam Woodcraft +43 more
TL;DR: In this paper, a sample of protostars and their spectral energy distributions were used to constrain key properties in the protostellar evolution, bolometric luminosity, and envelope mass and to build an evolutionary diagram.