Zobrazeno 1 - 10
of 69
pro vyhledávání: '"F. SIBILLE"'
Autor:
F. Sibille
Publikováno v:
MAB, Vol 25, Iss 7, Pp 266-273 (1951)
Externí odkaz:
https://doaj.org/article/2069e48168414bf9878c34baf06374e9
Publikováno v:
Médecine et Armées Vol. 44 No.4 ISBN: 9782813005076
Avec le conflit en Afghanistan, la reconnaissance ainsi que la prise en charge des blessures psychiques se sont améliorées. Cependant la rencontre avec la mort, événement traumatisant pourvoyeur de ces blessures, n’est pas l’apanage des Opér
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::eb0bf0d3323ac5709d2a16f89336bd3a
https://doi.org/10.17184/eac.6831
https://doi.org/10.17184/eac.6831
Autor:
F. Boulanger, P. Persi, Edith Falgarone, A. Coulais, C. J. Cesarsky, A. A. Kaas, Michel Perault, G. Olofsson, L. Nordh, E. Copet, F. Sibille, M. Huldtgren, Pascal André, T. Montmerle, Alain Abergel, Maryvonne Gerin, Jean-Loup Puget, M. M. Casali, Sylvain Bontemps, D. Teyssier, David Fosse, J. P. Bernard, John K. Davies
Publikováno v:
Astronomy & Astrophysics. 410:577-585
We present ISOCAM observations (5-18 µm) of the Horsehead nebula, together with observations of the (J = 1−0) and (J = 2−1) transitions of 12 CO, 13 CO and C 18 O taken at the IRAM 30-m telescope. The Horsehead nebula presents a typical photodis
Autor:
G. Olofsson, Anthony P. Jones, Alain Abergel, C. J. Cesarsky, John K. Davies, P. Persi, Edith Falgarone, M. M. Casali, M. Huldtgren, D. Cesarsky, T. Montmerle, L. Nordh, F. Sibille, M.-A. Miville-Deschenes, Pascal André, M. E. Copet, Michel Perault, A. A. Kaas, Jean-Loup Puget, Sylvain Bontemps, J. P. Bernard, F. Boulanger
Publikováno v:
Astronomy & Astrophysics. 389:239-251
We present ISOCAM observations (5 18 m) of the southern part of Orion B, including the reflection nebula NGC 2023 and the Horsehead nebula illuminated by the B star HD 37903 and the O star Orionis, respectively. Due to the limited radiation eld, the
Autor:
William T. Reach, Mark V. Sykes, Catherine Cesarsky, Francois Boulanger, John K. Davies, F. Sibille
Publikováno v:
Icarus. 127:251-254
We present the results of two scans through the dust trail of Comet P/Kopff made with ISOCAM on 26 March 1996. Positions behind the comet at mean anomalies of 0.5° and 1° less than the nucleus were imaged using the LW10 (IRAS Band 1, 12 μm) filter
Autor:
F. Sibille
Publikováno v:
Space Science Reviews. 74:225-228
I present the current status of arrays of detectors operating in the 1 – 200 micron range, restricted to mature devices, and two recent concepts of infrared detection which could lead to future developments.
Autor:
F. Billebaud, Emmanuel Lellouch, I. Vauglin, P. Merlin, Pierre Drossart, F. Sibille, B. Mosser, P. H. Lognonné
Publikováno v:
Geophysical Research Letters
Geophysical Research Letters, 1995, 22 (13), pp.1777-1780. ⟨10.1029/95GL01438⟩
Geophysical Research Letters, 1995, 22 (13), pp.1777-1780. ⟨10.1029/95GL01438⟩
We have observed Jupiter on July 24, 25, 26 and 27, 1994, in thermal infrared, using the French National 10 micron array camera “C10µ”, mounted on the Canada-France-Hawaii 3.6 meter telescope. The observations were made using both broad-band and
Akademický článek
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Autor:
Paolo Persi, Thierry Montmerle, M. M. Casali, Timo Prusti, A. A. Kaas, Edith Falgarone, P. Andre, Francois Boulanger, S. Olofsson, Magnus Gålfalk, Catherine Cesarsky, A. Abergel, John K. Davies, Göran Olofsson, L. Nordh, F. Sibille, Michel Perault, Sylvain Bontemps, Martin Burgdorf, J. L. Puget
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 420, pp.945-955. ⟨10.1051/0004-6361:20035758⟩
Astronomy and Astrophysics-A&A, 2004, 420, pp.945-955. ⟨10.1051/0004-6361:20035758⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 420, pp.945-955. ⟨10.1051/0004-6361:20035758⟩
Astronomy and Astrophysics-A&A, 2004, 420, pp.945-955. ⟨10.1051/0004-6361:20035758⟩
The results of a deep mid-IR ISOCAM survey of the L1551 dark molecular cloud are presented. The aim of this survey is a search for new YSO (Young Stellar Object) candidates, using two broad-band filters centred at 6.7 and 14.3 micron. Although two re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::70304d13774a7ab30672cb310f4b7e5b
Autor:
J. L. Puget, M. M. Casali, F. Boulanger, L. Nordh, Catherine Cesarsky, Göran Olofsson, Thierry Montmerle, Timo Prusti, A. Abergel, Frédérique Motte, M. Huldtgren, Sylvain Bontemps, A. A. Kaas, Martin Burgdorf, P. Andre, F. Sibille, Edith Falgarone, Michel Perault, Paolo Persi, Antonio Delgado, John K. Davies
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2004, 421, pp.623-642. ⟨10.1051/0004-6361:20035775⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 421, pp.623-642. ⟨10.1051/0004-6361:20035775⟩
Astronomy and Astrophysics-A&A, 2004, 421, pp.623-642. ⟨10.1051/0004-6361:20035775⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2004, 421, pp.623-642. ⟨10.1051/0004-6361:20035775⟩
We present results from an ISOCAM survey in the two broad band filters LW2 (5-8.5 mu) and LW3 (12-18 mu) of a 0.13 square degree coverage of the Serpens Main Cloud Core. A total of 392 sources were detected in the 6.7 mu band and 139 in the 14.3 mu b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::174016abda248f86c2750dd0d7a79d42
https://hal.science/hal-00009366
https://hal.science/hal-00009366