Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Ü. Kavak"'
Autor:
M. Tiwari, R. Kievit, S. Kabanovic, L. Bonne, F. Falasca, C. Guevara, R. Higgins, M. Justen, R. Karim, Ü. Kavak, C. Pabst, M. W. Pound, N. Schneider, R. Simon, J. Stutzki, M. Wolfire, A. G. G. M. Tielens
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 2, p 136 (2023)
We explore the potential of the Gaussian mixture model (GMM), an unsupervised machine-learning method, to identify coherent physical structures in the interstellar medium. The implementation we present can be used on any kind of spatially and spectra
Externí odkaz:
https://doaj.org/article/22a030c18d8c4584a4d40e1c5bac5510
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:
M. Tiwari, M. Wolfire, M. W. Pound, E. Tarantino, R. Karim, L. Bonne, C. Buchbender, R. Güsten, C. Guevara, S. Kabanovic, Ü. Kavak, M. Mertens, N. Schneider, R. Simon, J. Stutzki, A. G. G. M. Tielens
Publikováno v:
The Astronomical Journal, 164(4):150
We quantified the effects of stellar feedback in RCW 49 by determining the physical conditions in different regions using the [CII] 158 $\mu$m and [OI] 63 $\mu$m observations from SOFIA, the $^{12}$CO (3-2) observations from APEX and the H$_2$ line o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5292a0a47e40eb456c6587d36ca6959a
https://hdl.handle.net/1887/3514825
https://hdl.handle.net/1887/3514825
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