Zobrazeno 1 - 10
of 214
pro vyhledávání: '"Ph. André"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 520:4646-4663
We present the first analysis in NGC2071-North as a resolved hub-filament featuring a double centre. This $\sim 1.5 \times 1.5$ parsec-scale filament hub contains $\sim$500 $M_\odot$. Seen from Planck, magnetic field lines may have facilitated the ga
Akademický článek
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Akademický článek
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Publikováno v:
Astronomy & Astrophysics. 672:A133
Recent Herschel observations of nearby clouds have shown that filamentary structures are ubiquitous and that most prestellar cores form in filaments. Probing the density ($n$) and velocity ($V$) structure of filaments is crucial for the understanding
Publikováno v:
Astronomy & Astrophysics. 667:A90
We imaged the infrared dark clouds (IRDCs) G1.75-0.08 and G11.36+0.80 at 350 $\mu$m and 450 $\mu$m using the ArT\'eMiS bolometer. These data were used in conjunction with our previous 870 $\mu$m observations with the Large APEX BOlometer CAmera (LABO
Autor:
S. Anderl, B. Tabone, Anaëlle Maury, Arnaud Belloche, Frédéric Gueth, Ph. André, Sébastien Maret, Linda Podio, C. Codella, Sylvie Cabrit, Leonardo Testi, M. Gaudel, Bertrand Lefloch
Publikováno v:
Astronomy & Astrophysics, 648, 1-38
Aims. As a part of the CALYPSO Large Program, we aim to constrain the properties of protostellar jets and outflows by searching for corresponding emission in a sample of 21 Class 0 protostars covering a broad range of internal luminosities (Lint from
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70e20b37534d85517ec61be9eacb425d
https://ui.adsabs.harvard.edu/abs/2021A&A...648A..45P
https://ui.adsabs.harvard.edu/abs/2021A&A...648A..45P
Autor:
Arnaud Belloche, Linda Podio, S. Anderl, Claudio Codella, Frédéric Gueth, Aurore Bacmann, Sébastien Maret, Ph. André, Anaëlle Maury, S. Cabrit
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A123. ⟨10.1051/0004-6361/201936926⟩
Astronomy and Astrophysics-A&A, 2020, 643, pp.A123. ⟨10.1051/0004-6361/201936926⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 643, pp.A123. ⟨10.1051/0004-6361/201936926⟩
Astronomy and Astrophysics-A&A, 2020, 643, pp.A123. ⟨10.1051/0004-6361/201936926⟩
Context. The process of mass accretion in the earliest phases of star formation is still not fully understood: does the accretion rate smoothly decline with the age of the protostar or are there short, intermittent accretion bursts? The latter option
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d3d77e5a7446b80b4c003c3b929794b
https://hal.archives-ouvertes.fr/hal-03003699/file/aa36926-19.pdf
https://hal.archives-ouvertes.fr/hal-03003699/file/aa36926-19.pdf
Autor:
Vera Konyves, E. Fiorellino, Stefano Pezzuto, M. Benedettini, Derek Ward-Thompson, Frédérique Motte, Ph. André, Andrea Bracco, J. Di Francesco, Doris Arzoumanian, Jason M. Kirk, Sylvain Bontemps, Eugenio Schisano, Sergio Molinari, Davide Elia, Alexander Men'shchikov
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2020, ⟨10.1093/mnras/staa3420⟩
Monthly Notices of the Royal Astronomical Society: Letters, Oxford Journals, 2020, ⟨10.1093/mnras/staa3420⟩
The Herschel Gould Belt survey mapped the nearby (d < 500 pc) star-forming regions to understand better how the prestellar phase influences the star formation process. Here we report a complete census of dense cores in a 15 deg2 area of the Serpens s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3ebf8934c48830eaf6e5e1b3674d5e2a
http://arxiv.org/abs/2010.15241
http://arxiv.org/abs/2010.15241
Autor:
Stefano Pezzuto, Alexander Men'shchikov, Ph. André, J. Di Francesco, Christine D. Wilson, Sylvain Bontemps, L. Piccotti, Sarah Sadavoy, Frédérique Motte, Vera Konyves, P. Palmeirim, E. Fiorellino, Nicola Schneider, Jason M. Kirk, L. Spinoglio, Davide Elia, J.-Ph. Bernard, Eugenio Schisano, Doris Arzoumanian, G. Li Causi, M. Benedettini, Derek Ward-Thompson, Bilal Ladjelate
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A55. ⟨10.1051/0004-6361/201936534⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 645, pp.A55. ⟨10.1051/0004-6361/201936534⟩
(Abridged) In this paper, we present analyses of images taken with the Herschel ESA satellite from 70mu to 500mu. We first constructed column density and dust temperature maps. Next, we identified compact cores in the maps, and characterize the cores
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8b7f88d0a04cbebda5aaea7dbb59290b
http://arxiv.org/abs/2010.00006
http://arxiv.org/abs/2010.00006
Autor:
Nicolas Peretto, M. Figueira, Alexander Men'shchikov, Ph. André, Y. Shimajiri, D. Russeil, P. Palmeirim, Nicola Schneider, Vera Konyves, Annie Zavagno, H. Roussel, Timea Csengeri, S. N. Zhang, Gary A. Fuller, Frederic Schuller, Doris Arzoumanian
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A7. ⟨10.1051/0004-6361/202037815⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A7. ⟨10.1051/0004-6361/202037815⟩
Massive stars and their associated ionized (HII) regions could play a key role in the formation and evolution of filaments that host star formation. However, the properties of filaments that interact with H regions are still poorly known. To investig
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::71224a203613f99e370d70715cc8f75c