Zobrazeno 1 - 10
of 130
pro vyhledávání: '"LeLeu, G."'
Autor:
Figueira, M., Zavagno, A., Deharveng, L., Russeil, D., Anderson, L. D., Men'shchikov, A., Schneider, N., Hill, T., Motte, F., Mège, P., Leleu, G., Roussel, H., Bernard, J-P., Traficante, A., Paradis, D., Tigé, J., André, P., Bontemps, S., Abergel, A.
Publikováno v:
A&A 600, A93 (2017)
The expansion of HII regions can trigger the formation of stars. An overdensity of young stellar objects (YSOs) is observed at the edges of HII regions but the mechanisms that give rise to this phenomenon are not clearly identified. Moreover, it is d
Externí odkaz:
http://arxiv.org/abs/1612.08862
Autor:
Deharveng, L., Zavagno, A., Samal, M. R., Anderson, L. D., LeLeu, G., Brevot, D., Duarte-Cabral, A., Molinari, S., Pestalozzi, M., Foster, J. B., Rathborne, J. M., Jackson, J. M.
Publikováno v:
A&A 582, A1 (2015)
Our goal is to identify bipolar HII regions and to understand their morphology, their evolution, and the role they play in the formation of new generations of stars. We use the Spitzer and Herschel Hi-GAL surveys to identify bipolar HII regions. We s
Externí odkaz:
http://arxiv.org/abs/1507.00215
Autor:
Deharveng, L., Zavagno, A., Anderson, L. D., Motte, F., Abergel, A., Andre, Ph., Bontemps, S., Leleu, G., Roussel, H., Russeil, D.
W5-E has been observed with the Herschel-PACS and -SPIRE photometers, at 100, 160, 250, 350, and 500 microns. The dust temperature map shows a rather uniform temperature, in the range 17.5-20 K in the dense condensations or filaments, 21-22 K in the
Externí odkaz:
http://arxiv.org/abs/1209.2907
Akademický článek
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Autor:
Figueira, M., Zavagno, Annie, Deharveng, L., Russeil, D., Anderson, D., Men’shchikov, A., Schneider, N., Hill, T., Motte, F., Mège, P., Leleu, G., Roussel, H., Bernard, P., Traficante, A., Paradis, D., Tigé, J., André, P., Bontemps, Sylvain, Abergel, A., Anderson, L. D., Men'Shchikov, A., Bernard, J.-P.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 600, pp.id.A93. ⟨10.1051/0004-6361/201629379⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 600, pp.id.A93. 〈10.1051/0004-6361/201629379〉
Astronomy and Astrophysics-A&A, 2017, 600, pp.id.A93. ⟨10.1051/0004-6361/201629379⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 600, pp.id.A93. ⟨10.1051/0004-6361/201629379⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2017, 600, pp.id.A93. 〈10.1051/0004-6361/201629379〉
Astronomy and Astrophysics-A&A, 2017, 600, pp.id.A93. ⟨10.1051/0004-6361/201629379⟩
Context. The expansion of H ii regions can trigger the formation of stars. An overdensity of young stellar objects is observed at the edges of H ii regions but the mechanisms that give rise to this phenomenon are not clearly identified. Moreover, it
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2af4528ad47fc38a564c1dd059b764f
https://hal.archives-ouvertes.fr/hal-01509638/file/1612.08862.pdf
https://hal.archives-ouvertes.fr/hal-01509638/file/1612.08862.pdf
Akademický článek
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Publikováno v:
Astronomical Data Analysis Software and Systems XXI
Astronomical Data Analysis Software and Systems XXI, 2012, Unknown, Unknown Region. pp.885
Astronomical Data Analysis Software and Systems XXI, 2012, Unknown, Unknown Region. pp.885
International audience; We developed at CeSAM (Centre de donneeS Astrophysiques de Marseille) a new, Virtual Observatory compliant, Exposure Time Calculator, ETC-42. This new ETC performs an instrument-independent computation, derived from the compar
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::17401c0092d1dd79889072035b66f9e0
https://hal.archives-ouvertes.fr/hal-01437347
https://hal.archives-ouvertes.fr/hal-01437347
Autor:
Leleu, G., Méalier, A.-L., Benielli, D., Baluteau, J.-P., Surace, C., Fulton, T.~R., Imhof, P., Polehampton, E., Vibert, D.
Publikováno v:
Astronomical Data Analysis Software and Systems XXI
Astronomical Data Analysis Software and Systems XXI, 2012, Unknown, Unknown Region. pp.749
Astronomical Data Analysis Software and Systems XXI, 2012, Unknown, Unknown Region. pp.749
International audience; The Herschel Space Observatory is a cornerstone mission of the European Space Agency for astronomical observations in the far-infrared and sub-millimeter wavelength range (60 - 670 microns) and has been launched in May 2009 wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::7f9a22f7a044f202ceace7aca79d82f0
https://hal.archives-ouvertes.fr/hal-01428143
https://hal.archives-ouvertes.fr/hal-01428143
Publikováno v:
Astronomical Data Analysis Software and Systems XX
Astronomical Data Analysis Software and Systems XX, 2011, Unknown, Unknown Region. pp.559
Astronomical Data Analysis Software and Systems XX, 2011, Unknown, Unknown Region. pp.559
International audience; We developed at CeSAM (Centre de donnéeS Astrophysiques de Marseille) from LAM a new Virtual Observatory compliant Exposure Time Calculator. This new ETC has been designed to facilitate the integration of new sites, instrumen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3544857ffc576a263b883dd50e7da294
https://hal.archives-ouvertes.fr/hal-01437354
https://hal.archives-ouvertes.fr/hal-01437354
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.