Disruption of the Orion molecular core 1 by wind from the massive star θ

Autor: C, Pabst, R, Higgins, J R, Goicoechea, D, Teyssier, O, Berne, E, Chambers, M, Wolfire, S T, Suri, R, Guesten, J, Stutzki, U U, Graf, C, Risacher, A G G M, Tielens

Publikováno v: Nature. 565(7741)

Massive stars inject mechanical and radiative energy into the surrounding environment, which stirs it up, heats the gas, produces cloud and intercloud phases in the interstellar medium, and disrupts molecular clouds (the birth sites of new stars

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=pmid________::8ab4098a23d4790891e85c6018f35e20
https://pubmed.ncbi.nlm.nih.gov/30617315

Water in massive star-forming regions: HIFI observations of W3 IRS5

Autor: L. Chavarría, F. Herpin, T. Jacq, J. Braine, S. Bontemps, A. Baudry, M. Marseille, F. van der Tak, B. Pietropaoli, F. Wyrowski, R. Shipman, W. Frieswijk, E. F. van Dishoeck, J. Cernicharo, R. Bachiller, M. Benedettini, A. O. Benz, E. Bergin, P. Bjerkeli, G. A. Blake, S. Bruderer, P. Caselli, C. Codella, F. Daniel, A. M. di Giorgio, C. Dominik, S. D. Doty, P. Encrenaz, M. Fich, A. Fuente, T. Giannini, J. R. Goicoechea, Th. de Graauw, P. Hartogh, F. Helmich, G. J. Herczeg, M. R. Hogerheijde, D. Johnstone, J. K. Jørgensen, L. E. Kristensen, B. Larsson, D. Lis, R. Liseau, C. McCoey, G. Melnick, B. Nisini, M. Olberg, B. Parise, J. C. Pearson, R. Plume, C. Risacher, J. Santiago-García, P. Saraceno, J. Stutzki, R. Szczerba, M. Tafalla, A. Tielens, T. A. van Kempen, R. Visser, S. F. Wampfler, J. Willem, U. A. Yıldız

Publikováno v: Astronomy & astrophysics, 521:L37. EDP Sciences
Astronomy & Astrophysics, 521, L37
Astronomy & Astrophysics, 521:L37. EDP Sciences
Astronomy & Astrophysics, 521, pp. L37
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 521, pp.L37. ⟨10.1051/0004-6361/201015113⟩
Astronomy and Astrophysics-A&A, 2010, 521, pp.L37. ⟨10.1051/0004-6361/201015113⟩

We present Herschel observations of the water molecule in the massive star-forming region W3 IRS5. The o-H17O 110-101, p-H18O 111-000, p-H2O 22 202-111, p-H2O 111-000, o-H2O 221-212, and o-H2O 212-101 lines, covering a frequency range from 552 up to

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4b766c248ff040ea0fe6d4c5e06c1fc7
https://hdl.handle.net/11245/1.336616

Water abundances in high-mass protostellar envelopes: Herschel observations with HIFI

Autor: M. G. Marseille, F. F. S. van der Tak, F. Herpin, F. Wyrowski, L. Chavarría, B. Pietropaoli, A. Baudry, S. Bontemps, J. Cernicharo, T. Jacq, W. Frieswijk, R. Shipman, E. F. van Dishoeck, R. Bachiller, M. Benedettini, A. O. Benz, E. Bergin, P. Bjerkeli, G. A. Blake, J. Braine, S. Bruderer, P. Caselli, E. Caux, C. Codella, F. Daniel, P. Dieleman, A. M. di Giorgio, C. Dominik, S. D. Doty, P. Encrenaz, M. Fich, A. Fuente, T. Gaier, T. Giannini, J. R. Goicoechea, Th. de Graauw, F. Helmich, G. J. Herczeg, M. R. Hogerheijde, B. Jackson, H. Javadi, W. Jellema, D. Johnstone, J. K. Jørgensen, D. Kester, L. E. Kristensen, B. Larsson, W. Laauwen, D. Lis, R. Liseau, W. Luinge, C. McCoey, A. Megej, G. Melnick, D. Neufeld, B. Nisini, M. Olberg, B. Parise, J. C. Pearson, R. Plume, C. Risacher, P. Roelfsema, J. Santiago-García, P. Saraceno, P. Siegel, J. Stutzki, M. Tafalla, T. A. van Kempen, R. Visser, S. F. Wampfler, U. A. Yıldız

Publikováno v: Astronomy & Astrophysics, 521, L32
Astronomy & Astrophysics, 521. EDP Sciences
Astronomy & Astrophysics, 521, pp. L32
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 521, pp.L32. ⟨10.1051/0004-6361/201015103⟩
Astronomy & astrophysics, 521:L32. EDP Sciences

We derive the dense core structure and the water abundance in four massive star-forming regions which may help understand the earliest stages of massive star formation. We present Herschel-HIFI observations of the para-H2O 1_11-0_00 and 2_02-1_11 and

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::261633810447deef159d2385fa5dd989
https://hdl.handle.net/11245/1.336657

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