Zobrazeno 1 - 10
of 181
pro vyhledávání: '"S. Leurini"'
Autor:
A. Navarrini, L. Olmi, R. Nesti, P. Ortu, P. Marongiu, A. Orlati, A. Scalambra, A. Orfei, J. Roda, A. Cattani, S. Leurini, F. Govoni, M. Murgia, E. Carretti, D. Fierro, A. Pellizzoni
Publikováno v:
IEEE Access, Vol 10, Pp 26369-26403 (2022)
We report on the feasibility study of a W-band multibeam heterodyne receiver for the Sardinia Radio Telescope (SRT), a general purpose fully steerable 64-m diameter antenna located on the Sardinia island, Italy, managed by INAF (“Istituto Nazionale
Externí odkaz:
https://doaj.org/article/17f82700f2da47cdb44578e636364c2e
Autor:
F. Massi, A. Caratti o Garatti, R. Cesaroni, T. K. Sridharan, E. Ghose, E. Pinna, M. T. Beltrán, S. Leurini, L. Moscadelli, A. Sanna, G. Agapito, R. Briguglio, J. Christou, S. Esposito, T. Mazzoni, D. Miller, C. Plantet, J. Power, A. Puglisi, F. Rossi, B. Rothberg, G. Taylor, C. Veillet
We exploit the increased sensitivity of the recently installed AO SOUL at the LBT to obtain new high-spatial-resolution NIR images of the massive young stellar object IRAS20126+4104 and its outflow. We aim to derive the jet proper motions and kinemat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa82a7b86429a57bc5b3ea9fb56766f0
Autor:
K. R. Neralwar, D. Colombo, A. Duarte-Cabral, J. S. Urquhart, M. Mattern, F. Wyrowski, K. M. Menten, P. Barnes, Á. Sánchez-Monge, H. Beuther, A. J. Rigby, P. Mazumdar, D. Eden, T. Csengeri, C. L. Dobbs, V. S. Veena, S. Neupane, T. Henning, F. Schuller, S. Leurini, M. Wienen, A. Y. Yang, S. E. Ragan, S. Medina, Q. Nguyen-Luong
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142428⟩
Astronomy and Astrophysics-A&A, 2022, 663, ⟨10.1051/0004-6361/202142428⟩
We present one of the very first extensive classifications of a large sample of molecular clouds based on their morphology. This is achieved using a recently published catalogue of 10663 clouds obtained from the first data release of the SEDIGISM sur
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f84f40fd466f9e67960780e725d6f75
Autor:
A. R. Costa Silva, R. Fedriani, J. C. Tan, A. Caratti o Garatti, S. Ramsay, V. Rosero, G. Cosentino, P. Gorai, S. Leurini
Publikováno v:
Astronomy and Astrophysics
Massive stars form deeply embedded in their parental clouds, making it challenging to directly observe these stars and their immediate environments. It is known that accretion and ejection processes are intrinsically related, thus observing massive p
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9980ebf51f4dba8bf26b55bd2fcdce5f
http://arxiv.org/abs/2112.04463
http://arxiv.org/abs/2112.04463
Publikováno v:
Astronomy & Astrophysics, 658, A128
OB star clusters originate from parsec-scale massive molecular clumps. We aim to understand the evolution of temperature and density structures on the intermediate-scale ($\lesssim$0.1-1 pc) extended gas of massive clumps. We performed $\sim$0.1 pc r
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b00b95e1b8feeef87537138366778dd
http://arxiv.org/abs/2112.01115
http://arxiv.org/abs/2112.01115
Akademický článek
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Akademický článek
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Autor:
Carmelo Pino, G. Tudisco, Milena Benedettini, Renato Sortino, S. Leurini, Marco Molinaro, Ugo Becciani, Cristobal Bordiu, M. Raciti, Fabio Vitello, Filomena Bufano, D. Magro, Eva Sciacca, Simone Riggi
Publikováno v:
Astronomy and Computing
Innovative developments in data processing, archiving, analysis, and visualization are nowadays unavoidable to deal with the data deluge expected in next-generation facilities for radio astronomy, such as the Square Kilometre Array (SKA) and its prec
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2c48bf964c0b0de31a04eafeb5383e41
Autor:
Friedrich Wyrowski, Timea Csengeri, Th. Henning, H. Linz, S. Leurini, Pamela Klaassen, S. N. Longmore, Roberto Galván-Madrid, S. Suri, Siyi Feng, James Urquhart, Ralph E. Pudritz, Peter Schilke, C. Gieser, Vincent Piétu, J. M. Winters, D. Semenov, A. Ahmadi, Gary A. Fuller, Luke T. Maud, Thomas Peters, Stuart Lumsden, V. de Souza Magalhães, Álvaro Sánchez-Monge, Henrik Beuther, Qizhou Zhang, M. T. Beltrán, Rolf Kuiper, Aina Palau, Karl M. Menten, Luca Moscadelli, T. Möller, Jérôme Pety
Publikováno v:
Astronomy and Astrophysics, 648, 1-68
Aims. Current star formation research centers the characterization of the physical and chemical properties of massive stars, which are in the process of formation, at the spatial resolution of individual high-mass cores. Methods. We use sub-arcsecond
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::86865e7bbd5a69a6ae4fa55cffb39b0b
http://hdl.handle.net/20.500.12386/32477
http://hdl.handle.net/20.500.12386/32477
Autor:
Timea Csengeri, Leonardo Testi, Andrew Rigby, Karl M. Menten, S. J. Billington, V. S. Veena, Erik Muller, Friedrich Wyrowski, Alessio Traficante, M. T. Beltrán, Peter Schilke, S. Leurini, K. Torstensson, Jens Kauffmann, Toby J. T. Moore, M-Y Lee, Adam Ginsburg, P. Venegas, S-N X. Medina, Sylvain Bontemps, Frederic Schuller, D. Russeil, Leonardo Bronfman, Ke Wang, Sümeyye Suri, Riccardo Cesaroni, S. Lopez, David Eden, P. Mazumdar, F. Azagra, Th. Henning, Dario Colombo, Sarah Ragan, Jouni Kainulainen, P. J. Barnes, M. Wienen, M. Riener, Sergio Molinari, Álvaro Sánchez-Monge, Audra K. Hernandez, James Urquhart, A. Giannetti, F. M. Montenegro-Montes, Eugenio Schisano, Annie Zavagno, Rodrigo Parra, Frédérique Motte, M. Mattern, Alex R. Pettitt, Henrik Beuther, Clare Dobbs, Nicola Schneider, F. Mac-Auliffe, C. Agurto, E. Gonzalez, L. D. Anderson, Q. Nguyen-Luong, Ricardo Finger, J-P Perez-Beaupuits, Ana Duarte-Cabral
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.3064-3082. ⟨10.1093/mnras/staa2369⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2021, 500 (3), pp.3064-3082. ⟨10.1093/mnras/staa2369⟩
The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg^2 of the Galactic plane between l = -60 deg and l = +31 deg in several molecular transitions, including 13CO(2-1)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bc160a4e4b9d5d2bd0b80def20f8cd6a
https://hal.archives-ouvertes.fr/hal-03046462
https://hal.archives-ouvertes.fr/hal-03046462