Zobrazeno 1 - 10
of 33
pro vyhledávání: '"J. P. Pérez-Beaupuits"'
Autor:
J. R. Pardo, C. De Breuck, D. Muders, J. González, F. M. Montenegro-Montes, J. P. Pérez-Beaupuits, J. Cernicharo, C. Prigent, E. Serabyn, T. Mroczkowski, N. Phillips
8 pags., 5 figs.
Ground-based telescopes observing at millimeter (mm) and submillimeter (submm) wavelengths have to deal with a line-rich and highly variable atmospheric spectrum, both in space and time. Models of this spectrum play an important
Ground-based telescopes observing at millimeter (mm) and submillimeter (submm) wavelengths have to deal with a line-rich and highly variable atmospheric spectrum, both in space and time. Models of this spectrum play an important
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a454acb43197d42506eca91b2a637b15
https://api.elsevier.com/content/abstract/scopus_id/85141229251
https://api.elsevier.com/content/abstract/scopus_id/85141229251
Autor:
A. Beck, V. Lebouteiller, S. C. Madden, C. Iserlohe, A. Krabbe, L. Ramambason, C. Fischer, M. Kaźmierczak-Barthel, S. T. Latzko, J. P. Pérez-Beaupuits
Context. Massive star-formation leads to enrichment with heavy elements of the interstellar medium. On the other hand, the abundance of heavy elements is a key parameter to study the star-formation history of galaxies. Furthermore, the total molecula
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8a6f4f701a452cbc6d63afa405bd00f9
http://arxiv.org/abs/2206.15062
http://arxiv.org/abs/2206.15062
Autor:
Sarah Ragan, M. Riener, Nicola Schneider, M. T. Beltrán, L. D. Anderson, Ke Wang, S. N. X. Medina, S. Lopez, Andrew Rigby, Adam Ginsburg, P. Venegas, F. M. Montenegro-Montes, Frédérique Motte, Rodrigo Parra, Ricardo Finger, Annie Zavagno, M. Wienen, D. Russeil, Andrea Giannetti, Henrik Beuther, Karl M. Menten, Erik Muller, Álvaro Sánchez-Monge, C. Agurto, M. Mattern, Toby J. T. Moore, F. Mac-Auliffe, Silvia Leurini, Jens Kauffmann, Sergio Molinari, James Urquhart, V. S. Veena, Timea Csengeri, Alberto Sanna, P. Mazumdar, E. Gonzalez, L. Testi, Leonardo Bronfman, Min-Young Lee, Q. Nguyen-Luong, Ana Duarte-Cabral, Clare Dobbs, Jouni Kainulainen, Alessio Traficante, Peter Schilke, Th. Henning, Dario Colombo, J. P. Pérez-Beaupuits, Friedrich Wyrowski, K. Torstensson, Audra K. Hernandez, Sylvain Bontemps, Frederic Schuller, P. J. Barnes, Eugenio Schisano, David Eden, Riccardo Cesaroni, F. Azagra, Sümeyye Suri, Alex R. Pettitt
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
Monthly Notices of the Royal Astronomical Society, 2021, 500 (3), pp.3027-3049. ⟨10.1093/mnras/staa2480⟩
We use the 13CO(2-1) emission from the SEDIGISM high-resolution spectral-line survey of the inner Galaxy, to extract the molecular cloud population with a large dynamic range in spatial scales, using the SCIMES algorithm. This work compiles a cloud c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::60151acf5371e870a430a6cb82e292a9
http://arxiv.org/abs/2012.01502
http://arxiv.org/abs/2012.01502
Autor:
Karl M. Menten, M. Tiwari, W.-J. Kim, J. P. Pérez-Beaupuits, James Urquhart, Friedrich Wyrowski, Thushara Pillai
We study ten molecular transitions obtained from an unbiased 3 mm molecular line survey using the IRAM 30 m telescope toward 409 compact dust clumps identified by the APEX Telescope Large Area Survey of the Galaxy (ATLASGAL) to understand photodissoc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3dddafa4432705ef36bd237e5d979151
Akademický článek
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Autor:
Florian Kerber, Marc Sarazin, C. De Breuck, A. Wootten, J. P. Pérez-Beaupuits, Angel Otarola, Satoki Matsushita, L.-Å. Nyman, Tony Travouillon, Simon J. E. Radford
Atmospheric water vapor is the main limiting factor of atmospheric transparency in the mm and submm wavelength spectral windows. Thus, dry sites are needed for the installation and successful operation of radio astronomy observatories exploiting thos
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::84ca1f400005465c82f53540d65412ac
Autor:
Friedrich Wyrowski, J. P. Pérez-Beaupuits, Karl M. Menten, M. Tiwari, Min-Young Lee, W.-J. Kim
Hydrocarbons are ubiquitous in the interstellar medium, but their formation is still not well understood, depending on the physical environment they are found in. M8 is host to one of the brightest HII regions and PDRs in our galaxy. Using the APEX,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f736d79f45c7de3573bd3e6be975426d
Autor:
Friedrich Wyrowski, J. P. Pérez-Beaupuits, Karl M. Menten, W.-J. Kim, M.-Y. Lee, A. Giannetti, M. Tiwari
Publikováno v:
Astronomy & Astrophysics. 644:A25
Context. Messier 8 (M8), one of the brightest H II regions in our Galaxy, is powered by massive O-type stars and is associated with recent and ongoing massive star formation. Two prominent massive star-forming regions associated with M8 are M8-Main,
Autor:
Ronan Higgins, S. Bihr, C. Guevara, Volker Ossenkopf-Okada, J. Stutzki, R. Simon, Henrik Beuther, J. P. Pérez-Beaupuits, Urs U. Graf, Rolf Güsten
Publikováno v:
Astronomy & Astrophysics. 636:A16
Context. The [CII] 158 {\mu}m far-infrared (FIR) fine-structure line is one of the most important cooling lines of the star-forming interstellar medium (ISM). High spectral resolution observations have shown complex structures in the line profiles of
Autor:
Friedrich Wyrowski, Bernd Klein, Carsten Henkel, Karl M. Menten, M. Tiwari, J. P. Pérez-Beaupuits, Rolf Güsten, Helmut Wiesemeyer
Messier 8 is one of the brightest HII regions in the sky. Using SOFIA, APEX 12 m and IRAM 30 m telescopes, we have performed a comprehensive imaging survey of the emission from the [CII], [CI] and CO isotopologues within 1.3 $\times$ 1.3 pc around th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::02b865f03294e1e6ca54f14d22a8c1f4
http://arxiv.org/abs/1803.10164
http://arxiv.org/abs/1803.10164