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HOBYS and W43-HERO: Two more steps toward a Galaxy-wide understanding of high-mass star formation

Published online by Cambridge University Press:  12 September 2016

Frédérique Motte
Affiliation:
Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Univ. Grenoble Alpes - CNRS/INSU, BP 53, 38041 Grenoble Cedex 9, France email: [email protected] Laboratoire AIM Paris-Saclay, CEA/IRFU - CNRS/INSU - Univ. Paris Diderot, Service d'Astrophysique, Bât. 709, CEA-Saclay, F-91191 Gif-sur-Yvette Cedex, France
Sylvain Bontemps
Affiliation:
OASU/LAB-UMR 5804, CNRS - Université Bordeaux 1, 33270 Floirac, France
Jérémy Tigé
Affiliation:
Laboratoire dAstrophysique de Marseille (LAM), Aix Marseille Université - CNRS, UMR 7326, 13388, Marseille, France
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Abstract

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The Herschel/HOBYS key program allows to statistically study the formation of 10−20 M stars. The IRAM/W43-HERO large program is itself dedicated to the much more extreme W43 molecular complex, which forms stars up to 50 M. Both reveal high-density cloud filaments of several pc3, which are forming clusters of OB-type stars. Given their activity, these so-called mini-starburst cloud ridges could be seen as “miniature and instant models” of starburst galaxies. Both surveys also strongly suggest that high-mass prestellar cores do not exist, in agreement with the dynamical formation of cloud ridges. The HOBYS and W43 surveys are necessary steps towards Galaxy-wide studies of high-mass star formation.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2016 

References

André, Ph., Men'shchikov, A., Bontemps, , et al. 2010, A&A 518 L102 Google Scholar
Arzoumanian, D., André, Ph., Didelon, P., et al. 2011, A&A, 529, L6 Google Scholar
Bonnell, I. A. & Bate, M. R. 2006, MNRAS, 370, 488 Google Scholar
Bontemps, S., Motte, F., Csengeri, T., & Schneider, N. 2010, A&A, 524, A18 Google Scholar
Butler, M. J. & Tan, J. C. 2012, ApJ, 754, 5 Google Scholar
Csengeri, T., Bontemps, S., Schneider, N., Motte, F., & Dib, S. 2011a, A&A, 527, A135 Google Scholar
Csengeri, T., Bontemps, S., Schneider, N., et al. 2011b, ApJ, 740, L5 Google Scholar
Dale, J. E. & Bonnell, I. 2011, MNRAS, 414, 321 Google Scholar
Didelon, P., Motte, F., Tremblin, P. et al. 2015, A&A, 584, A4 Google Scholar
Duarte-Cabral, A., Bontemps, S., Motte, F., et al. 2013, A&A, 558, A125 Google Scholar
Duarte-Cabral, A., Bontemps, S., Motte, F., et al. 2014, A&A, 570, A1 Google Scholar
Elmegreen, B. 2011, in Star Formation in the Local Universe, EAS Pub. Series, 51, 45 Google Scholar
Federrath, C. & Klessen, R. S. 2012, ApJ, 761, 156 CrossRefGoogle Scholar
Federrath, C., Roman-Duval, J., Klessen, R. S., Schmidt, W., & Mac Low, M.-M. 2010, A&A, 512, A81 Google Scholar
Galván-Madrid, R., Zhang, Q., Keto, E., et al. 2010, ApJ, 725, 17 Google Scholar
Ginsburg, A., Bressert, E., Bally, J., & Battersby, C. 2012, ApJ, 758, L29 CrossRefGoogle Scholar
Hartmann, L., Ballesteros-Paredes, J., & Heitsch, F. 2012, MNRAS, 420, 1457 Google Scholar
Heitsch, F. & Hartmann, L. 2008, ApJ, 689, 290 Google Scholar
Hennebelle, P. & Chabrier, G. 2011, ApJ, 743, L29 Google Scholar
Hennemann, M., Motte, F., Schneider, N., et al. 2012, A&A, 543, L3 Google Scholar
Henshaw, J. D., Caselli, P., Fontani, F., Jimez-Serra, I., & Tan, J. C. 2014, MNRAS, 440, 2860 Google Scholar
Hill, T., Motte, F., Didelon, P., et al. 2011, A&A, 533, A9 Google Scholar
Hill, T., Motte, F., Didelon, P., et al. 2012, A&A, 542, A114 Google Scholar
Hosokawa, T. & Omukai, K. 2009, ApJ, 691, 823 Google Scholar
Könyves, V., André, Ph., Men'shchikov, A., et al. 2015, A&A, 584, A91 Google Scholar
Kroupa, P. 2001, MNRAS, 322, 231 Google Scholar
Krumholz, M. 2014, Physics Reports 539 Iss. 2, 49134 Google Scholar
Krumholz, M. R. & McKee, C. F. 2005, ApJ, 630, 250 Google Scholar
Louvet, F., Motte, F., Hennebelle, P., et al. 2014, A&A 570 A15 Google Scholar
Louvet, F., Motte, F., Gusdorf, A., et al. 2016, soon to be submitted to A&A Google Scholar
McKee, C. F. & Tan, J. C. 2002, Nature, 416, 59 Google Scholar
Menshchikov, A., André, P., Didelon, P., et al. 2012, A&A, 542, A81 Google Scholar
Minier, V., Tremblin, P., Hill, T., et al. 2013, A&A, 550, A50 Google Scholar
Motte, F. & André, Ph. 2001, A&A, 365, 440 Google Scholar
Motte, F., André, Ph., & Neri, R. 1998, A&A, 336, 150 Google Scholar
Motte, F., Bontemps, S., Schilke, P., et al. 2007, A&A 476 1243 Google Scholar
Motte, F., Schilke, P., & Lis, D. C. 2003, ApJ, 582, 277 CrossRefGoogle Scholar
Motte, F., Zavagno, A., Bontemps, S., et al. 2010, A&A 518 L77 Google Scholar
Nguyen Luong, Q., Motte, F., Carlhoff, P., et al. 2013, ApJ, 775, 88 Google Scholar
Nguyen Luong, Q., Motte, F., Hennemann, M., et al. 2011a, A&A, 535, A76 Google Scholar
Nguyen Luong, Q., Motte, F., Schuller, F., et al. 2011b, A&A 529 A41 Google Scholar
Padoan, P. & Nordlund, A. 2011, ApJ, 730, 40 Google Scholar
Peretto, N., Fuller, G. A., Duarte-Cabral, A., et al. 2013, A&A, 555, A112 Google Scholar
Russeil, D., Zavagno, A., Motte, F., et al. 2010, A&A 515 A55 Google Scholar
Schneider, N., Csengeri, T., Bontemps, S., et al. 2010a, A&A 520 A49 Google Scholar
Schneider, N., Csengeri, T., Hennemann, M., et al. 2012, A&A, 540, L11 Google Scholar
Tan, J. C., Kong, S., Butler, M. J., Caselli, P., & Fontani, F. 2013, ApJ, 779, 96 Google Scholar
Tigé, J., Motte, F., Russeil, , et al. 2016, soon to be submitted to A&A Google Scholar
Tremblin, P., Audit, E., Minier, V., Schmidt, W., & Schneider, N. 2012, A&A, 546, A33 Google Scholar
Vázquez-Semadeni, E., Kim, J., & Ballesteros-Paredes, J. 2005, ApJ, 630, L49 Google Scholar
Vázquez-Semadeni, E., González, R. F., Ballesteros-Paredes, J., Gazol, A., & Kim, J. 2008, MNRAS, 390, 769 Google Scholar