Pre- A nd protostellar cores in the Rosette Nebula

R. Bögner, T. Csengeri, M. Wienen, N. Schneider, J. Montillaud, L. V. Tóth, Bruce G. Elmegreen, L. Viktor Tóth, Manuel Güdel

Research output: Contribution to journalArticle

Abstract

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- A nd 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.

Original languageEnglish
Pages (from-to)371-372
Number of pages2
JournalProceedings of the International Astronomical Union
DOIs
Publication statusAccepted/In press - 2019

Keywords

  • radio lines: ISM
  • stars: Formation

ASJC Scopus subject areas

  • Medicine (miscellaneous)
  • Astronomy and Astrophysics
  • Nutrition and Dietetics
  • Public Health, Environmental and Occupational Health
  • Space and Planetary Science

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    Bögner, R., Csengeri, T., Wienen, M., Schneider, N., Montillaud, J., Tóth, L. V., Elmegreen, B. G., Tóth, L. V., & Güdel, M. (Accepted/In press). Pre- A nd protostellar cores in the Rosette Nebula. Proceedings of the International Astronomical Union, 371-372. https://doi.org/10.1017/S1743921319002254