Hostname: page-component-78c5997874-ndw9j Total loading time: 0 Render date: 2024-11-03T00:02:42.628Z Has data issue: false hasContentIssue false

Pre- and protostellar cores in the Rosette Nebula

Published online by Cambridge University Press:  13 January 2020

R. Bögner
Affiliation:
Department of Astronomy, Eötvös Loránd University, 1/A Pázmány Péter sétány, 1117 Budapest, Hungary email: [email protected]
T. Csengeri
Affiliation:
Max-Planck-Institut für Radioastronomie, 69 Auf dem Hügel, 53121 Bonn, Germany
M. Wienen
Affiliation:
College of Engineering, Mathematics and Physical Sciences, University of Exeter, North Park Road, EX4 4QL Exeter, UK
N. Schneider
Affiliation:
I. Physikalische Institut, University of Cologne, 77 Zuelpicher Str., 50937 Cologne, Germany
J. Montillaud
Affiliation:
Institut Utinam, CNRS UMR 6213, OSU THETA, Université de Franche-Comté, 41 bis avenue de l’Observatoire, 25000 Besançon, France
L. V. Tóth
Affiliation:
Department of Astronomy, Eötvös Loránd University, 1/A Pázmány Péter sétány, 1117 Budapest, Hungary email: [email protected] Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, 15-17 Konkoly-Thege Mikló út, 1121, Budapest, Hungary
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Recent theories on the formation of the Solar System turned the attention to the study of low mass cloud cores in massive star forming regions. The Rosette Molecular Cloud is a well-known star forming area having highly filamentary structure with dense cores covering a wide range of masses. These pre- and protostellar cores were observed by Herschel and key core properties were derived from its data. With the Effelsberg 100m telescope a sample of these cores with masses ranging between 3-40 M were observed in ammonia inversion lines. In this work we are examining the correlations between these two datasets with the aim of gaining insight of the processes behind the star formation of the region.

Type
Contributed Papers
Copyright
© International Astronomical Union 2020 

References

Sridharan, T. K., Beuther, H., Saito, M., Wyrowsky, F., & Schilke, P. 2005, ApJ, 634L, 57S CrossRefGoogle Scholar
Motte, F., Zavagno, A., Bontemps, S., et al. 2010, A&A, 518, L77 Google Scholar
Hennemann, F., Motte, F., Bontemps, S. et al. 2010, A&A, 518, L84 Google Scholar
Schneider, N., Motte, F., Bontemps, S. et al. 2010, A&A, 518, L83 Google Scholar
Wienen, M., Wyrowski, F., Schuller, et al. 2012, A&A, 544, A146 Google Scholar
Cambrésy, L., Marton, G., Fehér, O., Tóth, L. V., Schneider, N. 2013, A&A, 557, A29 Google Scholar
Montillaud, J., Juvela, M., Rivera-Ingraham, A. et al. 2015, A&A, 584, A92 Google Scholar