Zobrazeno 1 - 10
of 261
pro vyhledávání: '"H. A. Pabst"'
Autor:
Ü. Kavak, J. Bally, J. R. Goicoechea, C. H. M. Pabst, F. F. S. van der Tak, A. G. G. M. Tielens
Publikováno v:
Astronomy & Astrophysics, 663:A117
Astronomy and astrophysics, 663:A117. EDP Sciences
Astronomy and astrophysics, 663:A117. EDP Sciences
17 pags., 18 figs., 3 tabs.
Context. Interest in stellar feedback has recently increased because new studies suggest that radiative and mechanical feedback from young massive stars significantly regulates the physical and chemical composition of
Context. Interest in stellar feedback has recently increased because new studies suggest that radiative and mechanical feedback from young massive stars significantly regulates the physical and chemical composition of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5ae315d925abe68ac71001355f8bc9d
Autor:
Ü. Kavak, J. R. Goicoechea, C. H. M. Pabst, J. Bally, F. F. S. van der Tak, A. G. G. M. Tielens
Publikováno v:
Astronomy and astrophysics, 660:A109. EDP Sciences
Astronomy & Astrophysics, 660:A109
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 660:A109
Digital.CSIC. Repositorio Institucional del CSIC
instname
20 pags., 20 figs., 2 tabs.
Context. The role of feedback in the self-regulation of star formation is a fundamental question in astrophysics. The Orion Nebula is the nearest site of ongoing and recent massive star formation. It is a unique labor
Context. The role of feedback in the self-regulation of star formation is a fundamental question in astrophysics. The Orion Nebula is the nearest site of ongoing and recent massive star formation. It is a unique labor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7205eacf8df3b7ee7438c29c2a8e4439
https://doi.org/10.1051/0004-6361/202141367
https://doi.org/10.1051/0004-6361/202141367
Autor:
R. Güsten, S. Kabanovic, Ronan Higgins, Mark G. Wolfire, O. Berne, Aggm Tielens, J. R. Goicoechea, D. Teyssier, C. H. M. Pabst, J. Stutzki, E. Chambers, C. Kramer, Alvaro Hacar
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 658, ⟨10.1051/0004-6361/202140805⟩
Astronomy & Astrophysics, 658:A98
Astronomy and Astrophysics-A&A, 2022, 658, ⟨10.1051/0004-6361/202140805⟩
Astronomy & Astrophysics, 658:A98
34 pags., 34 figs., 15 tabs.
Context. The [C II] 158 m fine-structure line is the dominant cooling line of moderate-density photodissociation regions (PDRs) illuminated by moderately bright far-ultraviolet (FUV) radiation fields. This makes this
Context. The [C II] 158 m fine-structure line is the dominant cooling line of moderate-density photodissociation regions (PDRs) illuminated by moderately bright far-ultraviolet (FUV) radiation fields. This makes this
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::224e8b905da3c9f07c8dd3fea477f55a
https://hal-insu.archives-ouvertes.fr/insu-03672056/file/aa40805-21.pdf
https://hal-insu.archives-ouvertes.fr/insu-03672056/file/aa40805-21.pdf
Autor:
Rolf Güsten, S. Suri, Olivier Berné, S. Kabanovic, Mark G. Wolfire, Alexander G. G. M. Tielens, C. H. M. Pabst, Ronan Higgins, Javier R. Goicoechea, Yoko Okada, Heiko Richter, A. Parikka, Juergen Stutzki, E. Chambers, D. Teyssier, Christof Buchbender, M. Mertens, Rebeca Aladro
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 652, 1-23
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 652, ⟨10.1051/0004-6361/202039621⟩
instname
Astronomy & Astrophysics, 652, 1-23
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2021, 652, ⟨10.1051/0004-6361/202039621⟩
24 pags., 32 figs., 3 tabs.
Context. The [CII] 158 μm far-infrared fine-structure line is one of the dominant cooling lines of the star-forming interstellar medium. Hence [CII] emission originates in and thus can be used to trace a range of ISM
Context. The [CII] 158 μm far-infrared fine-structure line is one of the dominant cooling lines of the star-forming interstellar medium. Hence [CII] emission originates in and thus can be used to trace a range of ISM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::140ab9d7f51b5a7fa5cd2236ceb6ee7f
http://arxiv.org/abs/2106.15620
http://arxiv.org/abs/2106.15620
Autor:
Oliver Ricken, Christof Buchbender, C. H. M. Pabst, Robert Simon, Mark G. Wolfire, A. G. G. M. Tielens, Arshia M. Jacob, R. Higgins, Rolf Güsten, R. Karim, Nicola Schneider, C. Guevara, S. Kabanovic, M. Tiwari, Marc W. Pound, Juergen Stutzki
Publikováno v:
The Astrophysical Journal, 914(2)
We unveil the stellar wind driven shell of the luminous massive star-forming region of RCW 49 using SOFIA FEEDBACK observations of the [CII] 158 $\mu$m line. The complementary dataset of the $^{12}$CO and $^{13}$CO J = 3 - 2 transitions is observed b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::834215f978e8209be29a04e512bc24e6
http://arxiv.org/abs/2104.04276
http://arxiv.org/abs/2104.04276
Autor:
Aggm Tielens, C. H. M. Pabst, Henrik Beuther, Nicolas Reyes, Urs U. Graf, O. Ricken, Annie Zavagno, Heiko Richter, Karl M. Menten, Bhaswati Mookerjea, Helmut Wiesemeyer, R. Simon, M. Justen, Mark Wolfire, S. Kabanovic, L. D. Anderson, Antoine Gusdorf, Matteo Luisi, L. Bonne, Ronan Higgins, Christof Buchbender, K. Jacobs, John Bally, Friedrich Wyrowski, Yoko Okada, Markus Röllig, Timea Csengeri, R. Karim, M. Mertens, G. Sandell, Marc W. Pound, Volker Ossenkopf-Okada, J. Stutzki, M. Tiwari, E. Chambers, D. Russeil, Álvaro Sánchez-Monge, Rolf Güsten, Nicola Schneider, Sylvain Bontemps, C. Guevara
Publikováno v:
Publications of the Astronomical Society of the Pacific, 132(1016), 104301
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2020, 132 (1016), pp.104301. ⟨10.1088/1538-3873/aba840⟩
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2020, 132 (1016), pp.104301. ⟨10.1088/1538-3873/aba840⟩
FEEDBACK is a SOFIA (Stratospheric Observatory for Infrared Astronomy) legacy program dedicated to study the interaction of massive stars with their environment. It performs a survey of 11 galactic high mass star-forming regions in the 158 μm (1.9 T
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::98405c1780fe0cfcc20580f8e2f2acbe
https://elib.dlr.de/136959/
https://elib.dlr.de/136959/
Autor:
S. Kabanovic, Ronan Higgins, Olivier Berné, Rolf Güsten, Javier R. Goicoechea, C. H. M. Pabst, Aggm Tielens, D. Teyssier, J. Stutzki, E. Chambers
Publikováno v:
Astronomy & Astrophysics, 639, A2
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, ⟨10.1051/0004-6361/202037560⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, ⟨10.1051/0004-6361/202037560⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
26 pags., 33 figs., 10 tabs.
Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive stars have profound effects on their environment due to their strong radiation fields and stellar winds. Stellar feedback is one
Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive stars have profound effects on their environment due to their strong radiation fields and stellar winds. Stellar feedback is one
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3fda5c0f379d3a5cabb7514da143aff8
https://ui.adsabs.harvard.edu/abs/2020A&A...639A...2P
https://ui.adsabs.harvard.edu/abs/2020A&A...639A...2P
Autor:
S. Suri, S. Kabanovic, C. Kramer, Nuria Marcelino, Alvaro Hacar, Aggm Tielens, C. H. M. Pabst, Ronan Higgins, Javier R. Goicoechea, D. Teyssier, S. Cuadrado, Olivier Berné, Mark G. Wolfire, J. Stutzki, M. G. Santa-Maria, Christof Buchbender
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy & Astrophysics, 639, A1
instname
Astronomy & Astrophysics, 639, A1
18 pags., 21 figs., 5 tabs, 1 app.
Strong winds and ultraviolet (UV) radiation from O-type stars disrupt and ionize their molecular core birthplaces, sweeping up material into parsec-size shells. Owing to dissociation by starlight, the thinnest
Strong winds and ultraviolet (UV) radiation from O-type stars disrupt and ionize their molecular core birthplaces, sweeping up material into parsec-size shells. Owing to dissociation by starlight, the thinnest
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9649aac05c6ac0e548acda069a40ad0
http://hdl.handle.net/10261/219254
http://hdl.handle.net/10261/219254
Autor:
J. B. R. Oonk, A. G. G. M. Tielens, M. C. Toribio, H. J. A. Röttgering, C. H. M. Pabst, K. L. Emig, P. Salas
Publikováno v:
Astronomy and Astrophysics (0004-6361), 626, A70
Context. The combined use of carbon radio recombination lines (CRRLs) and the 158 $\mu$m-[CII] line is a powerful tool for the study of the energetics and physical conditions (e.g., temperature and density) of photodissociation regions (PDRs). Howeve
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::743503b423e555c0fe54939aab2f0953
https://hdl.handle.net/1887/83178
https://hdl.handle.net/1887/83178
Autor:
D. Teyssier, Rolf Guesten, Urs U. Graf, J. R. Goicoechea, A. G. G. M. Tielens, J. Stutzki, E. Chambers, O. Berne, Ronan Higgins, Christophe Risacher, C. H. M. Pabst, Mark Wolfire, Sümeyye Suri
Publikováno v:
Nature, 565(7741), 618-621
Digital.CSIC. Repositorio Institucional del CSIC
instname
Digital.CSIC. Repositorio Institucional del CSIC
instname
16 pags., 9 figs., 1 tab.
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 (th
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 (th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fd296c2ed08cda488cc38922d727d3be
http://hdl.handle.net/10261/207570
http://hdl.handle.net/10261/207570
