Zobrazeno 1 - 10 of 120 pro vyhledávání: '"J.‐P. Baluteau"'
1
$Herschel$ SPIRE-FTS observations of RCW 120
Autor: Alain Abergel, F. Le Petit, J.-P. Baluteau, J. A. Rodón, M. Köhler, Annie Zavagno, Emilie Habart, J. Le Bourlot
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2015, 579
The expansion of Galactic HII regions can trigger the formation of a new generation of stars. However, little is know about the physical conditions that prevail in these regions. We study the physical conditions that prevail in specific zones towards
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d3f5f08cfcec584d920aaacfb72d46a
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2
Infrared Space ObservatoryLong Wavelength Spectrometer Observations of C+and O0Lines in Absorption toward Sagittarius B2
Autor: C. Vastel, E. T. Polehampton, J.‐P. Baluteau, B. M. Swinyard, E. Caux, P. Cox
Publikováno v: The Astrophysical Journal. 581:315-324
High spectral resolution Fabry-P erot observations of the [O I] 63.2 and 145.5 ma nd [CII] 157.7 m ne structure lines are presented for the center of the Sagittarius B2 complex (Sgr B2). The data were obtained with the Long Wavelength Spectrometer on
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::2560404598e14c3125c3e9189c6e8b13
https://doi.org/10.1086/344136
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3
The physical structure of Magellanic Cloud HII regions I. Dataset
Autor: F Damour, J. M. van der Hulst, R. Vermeij, J.-P. Baluteau
Publikováno v: Astronomy & astrophysics, 390(2), 649-665. EDP Sciences
We present infrared and optical spectroscopic data for 11 H II regions and one Supernova Remnant in the Large and Small Magellanic Cloud. The infrared data have been obtained with the Short Wavelength Spectrometer and Long Wavelength Spectrometer on
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f77569e1098095e2886405c8440fb372
https://doi.org/10.1051/0004-6361:20020424
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4
Detection of HD in emission towards Sagittarius B2
Autor: J.-P. Baluteau, Bruce Swinyard, Emmanuel Caux, Cecilia Ceccarelli, Edward Polehampton
Publikováno v: Astronomy & Astrophysics. 388:L44-L47
The giant molecular cloud Sagittarius B2, located near the Galactic Centre, has been observed in the far-infrared by the ISO Long Wavelength Spectrometer. Wavelengths in the range 47-196 microns were covered with the high resolution Fabry-Perot spect
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bcf9b61b29825bdf45685376bf0fb691
https://doi.org/10.1051/0004-6361:20020630
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5
A photoionization model of the compact HII region G29.96-0.02
Autor: N. L. Martin-Hernandez, Els Peeters, Christophe Morisset, Pieter R. Roelfsema, J. P. Baluteau, Daniel Schaerer, F. Damour, Pierre Cox
Publikováno v: Astronomy & astrophysics, 386(2), 558-570. EDP Sciences
We present a detailed photoionization model of G29.96-0.02 (hereafter G29.96), one of the brightest Galactic Ultra Compact HII (UCHII) regions in the Galaxy. This source has been observed extensively at radio and infrared wavelengths. The most recent
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::97ae57a2433c3c002709e1eaa3fed46b
https://research.rug.nl/en/publications/16e70f2f-4d6d-4f2b-92e5-40025a8f5b61
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6
ISO ammonia line absorption reveals a layer of hot gas veiling Sgr B2
Autor: Bruce Swinyard, M. F. Kessler, Malcolm Walmsley, Cecile Gry, Timo Prusti, Emmanuel Caux, Pierre Cox, Sunil Sidher, Cecilia Ceccarelli, J.-P. Baluteau
Publikováno v: Astronomy & Astrophysics. 383:603-613
We report the rst results of the unbiased spectral high resolution survey obtained towards Sgr B2 with the Long Wavelength Spectrometer on board ISO. The survey detected more than one hundreds lines from several molecules. Ammonia is the molecule wit
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::8b491afa2aa3068102d5427da2944266
https://doi.org/10.1051/0004-6361:20011765
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7
Initial highlights of the HOBYS key program, the Herschel imaging survey of OB young stellar objects
Autor: Annie Zavagno, Nicola Schneider, Sergio Molinari, Jason M. Kirk, Pierre Didelon, Timea Csengeri, Zoltan Balog, L. D. Anderson, Matthew Joseph Griffin, D. Russeil, Peter Charles Hargrave, S. J. Leeks, Adam Woodcraft, Marc Sauvage, Christine D. Wilson, Alain Abergel, M. Hennemann, Q. Nguyen-Luong, Vincent Minier, Maohai Huang, J.-P. Baluteau, D. Teyssier, Pierrick Martin, Lise Deharveng, Alexander Men'shchikov, P. Persi, Derek Ward-Thompson, H. Roussel, Glenn J. White, Ph. André, Sylvain Bontemps, Leonardo Testi, S. Sadavoy, Pierre Cox, A. M. di Giorgio, Tracey Hill, R. Vavrek, Stefano Pezzuto, Luigi Spinoglio, Frédérique Motte, P. Saraceno, G. Olofsson, A. Marston, H. Aussel, Jin-Zeng Li, B. Sibthorpe, J. Di Francesco, J.-Ph. Bernard, Nicolas Peretto
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, pp.L77. ⟨10.1051/0004-6361/201014690⟩
Astronomy and Astrophysics-A&A, 2010, 518, pp.L77. ⟨10.1051/0004-6361/201014690⟩
Scopus-Elsevier
International audience; We present the initial highlights of the HOBYS key program, which are based on Herschel images of the Rosette molecular complex and maps of the RCW120 H ii region. Using both SPIRE at 250/350/500 μm and PACS at 70/160 μm or
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::612963b7ad81dd65f1f7bfb05f19b6fb
https://hal.archives-ouvertes.fr/hal-00526246/document
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8
Herschel-SPIRE observations of the Polaris flare : structure of the diffuse interstellar medium at the sub-parsec scale
Autor: M.-A. Miville-Deschênes, P. G. Martin, A. Abergel, J.-P. Bernard, F. Boulanger, G. Lagache, L. D. Anderson, P. André, H. Arab, J.-P. Baluteau, K. Blagrave, S. Bontemps, M. Cohen, M. Compiegne, P. Cox, E. Dartois, G. Davis, R. Emery, T. Fulton, C. Gry, E. Habart, M. Huang, C. Joblin, S. C. Jones, J. Kirk, T. Lim, S. Madden, G. Makiwa, A. Menshchikov, S. Molinari, H. Moseley, F. Motte, D. A. Naylor, K. Okumura, D. Pinheiro Gonçalves, E. Polehampton, J. A. Rodón, D. Russeil, P. Saraceno, N. Schneider, S. Sidher, L. Spencer, B. Swinyard, D. Ward-Thompson, G. J. White, A. Zavagno
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, pp.L104. ⟨10.1051/0004-6361/201014678⟩
Astronomy and Astrophysics-A&A, 2010, 518, pp.L104. ⟨10.1051/0004-6361/201014678⟩
We present a power spectrum analysis of the Herschel-SPIRE observations of the Polaris flare, a high Galactic latitude cirrus cloud midway between the diffuse and molecular phases. The SPIRE images of the Polaris flare reveal for the first time the s
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3422a60d59dbb2be0106c75f249b396a
https://hal.archives-ouvertes.fr/hal-00523050
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9
The Herschel first look at protostars in the Aquila Rift
Autor: Matthew Joseph Griffin, Adam Woodcraft, Marc Sauvage, Stefano Pezzuto, Vera Könyves, Bruce Sibthorpe, Frédérique Motte, Vincent Minier, Doris Arzoumanian, Pierre Cox, Peter Charles Hargrave, P. Didelon, Nicolas Peretto, Annie Zavagno, Alexander Men'shchikov, J.-Ph. Bernard, Glenn J. White, Ph. André, Leonardo Testi, Bruno Merín, J. Di Francesco, Göran Olofsson, C. D. Wilson, R. Vavrek, M. Attard, Alain Abergel, Sylvain Bontemps, Maohai Huang, A. M. Di Giorgo, J.-P. Baluteau, Timo Prusti, P. Saraceno, Nicola Schneider, Jason M. Kirk, Anaëlle Maury, Derek Ward-Thompson, Peter Martin, Jin-Zeng Li, Sergio Molinari, Helene Roussel, D. Russeil, L. Spinoglio, L. Cambrésy
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, pp.L85. ⟨10.1051/0004-6361/201014661⟩
Astronomy and Astrophysics-A&A, 2010, 518, pp.L85. ⟨10.1051/0004-6361/201014661⟩
Scopus-Elsevier
As part of the science demonstration phase of the Herschel mission of the Gould Belt Key Program, the Aquila Rift molecular complex has been observed. The complete ~ 3.3deg x 3.3deg imaging with SPIRE 250/350/500 micron and PACS 70/160 micron allows
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bebbfe9fdebce9a87e7b9165a413f352
https://hal.archives-ouvertes.fr/hal-00523476
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10
First detection of the methylidyne cation (CH+) fundamental rotational line with the Herschel/SPIRE FTS
Autor: D. A. Naylor, E. Dartois, E. Habart, A. Abergel, J.-P. Baluteau, S. C. Jones, E. Polehampton, P. Ade, L. D. Anderson, P. André, H. Arab, J.-P. Bernard, K. Blagrave, S. Bontemps, F. Boulanger, M. Cohen, M. Compiègne, P. Cox, G. Davis, R. Emery, T. Fulton, C. Gry, M. Huang, C. Joblin, J. M. Kirk, G. Lagache, T. Lim, S. Madden, G. Makiwa, P. Martin, M.-A. Miville-Deschênes, S. Molinari, H. Moseley, F. Motte, K. Okumura, D. Pinheiro Gonçalves, J. A. Rodón, D. Russeil, P. Saraceno, S. Sidher, L. Spencer, B. Swinyard, D. Ward-Thompson, G. J. White, A. Zavagno
Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2010, 518, pp.L117. ⟨10.1051/0004-6361/201014656⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2010, 518, pp.L117. ⟨10.1051/0004-6361/201014656⟩
Aims. To follow the species chemistry arising in diverse sources of the Galaxy with Herschel. Methods. SPIRE FTS sparse sampled maps of the Orion bar & compact HII regions G29.96-0.02 and G32.80+0.19 have been analyzed. Results. Beyond the wealth of
Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b43a20d70f52f0b6daa48c9190400d00
https://hal.science/hal-00522987
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