Zobrazeno 1 - 10
of 2 254
pro vyhledávání: '"d'Hendecourt, L"'
Autor:
Urso, R. G., Vuitton, V., Danger, G., d'Hendecourt, L. Le Sergeant, Flandinet, L., Djouadi, Z., Mivumbi, O., Orthous-Daunay, F. R., Ruf, A., Vinogradoff, V., Wolters, C., Brunetto, R.
Publikováno v:
A&A 644, A115 (2020)
Context. Near- and mid-infrared observations have revealed the presence of organic refractory materials in the solar system, in cometary nuclei and on the surface of centaurs, Kuiper-belt and trans-neptunian objects. In these astrophysical environmen
Externí odkaz:
http://arxiv.org/abs/2011.08650
Autor:
Merlin, Francesca
Publikováno v:
Tecnoscienza. Italian Journal of Science & Technology Studies
Tecnoscienza. Italian Journal of Science & Technology Studies, STS Italia, 2015, 6 (2), pp.176-181
Tecnoscienza. Italian Journal of Science & Technology Studies, STS Italia, 2015, 6 (2), pp.176-181
International audience
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::cff73f3a56ddbbaeb37e8edc4d0184ce
https://hal.archives-ouvertes.fr/hal-01455184
https://hal.archives-ouvertes.fr/hal-01455184
Autor:
Mousis, O., Atkinson, D. H., Cavalié, T., Fletcher, L. N., Amato, M. J., Aslam, S., Ferri, F., Renard, J. -B., Spilker, T., Venkatapathy, E., Wurz, P., Aplin, K., Coustenis, A., Deleuil, M., Dobrijevic, M., Fouchet, T., Guillot, T., Hartogh, P., Hewagama, T., Hofstadter, M. D., Hue, V., Hueso, R., Lebreton, J. -P., Lellouch, E., Moses, J., Orton, G. S., Pearl, J. C., Sanchez-Lavega, A., Simon, A., Venot, O., Waite, J. H., Achterberg, R. K., Atreya, S., Billebaud, F., Blanc, M., Borget, F., Brugger, B., Charnoz, S., Chiavassa, T., Cottini, V., d'Hendecourt, L., Danger, G., Encrenaz, T., Gorius, N. J. P., Jorda, L., Marty, B., Moreno, R., Morse, A., Nixon, C., Reh, K., Ronnet, T., Schmider, F. -X., Sheridan, S., Sotin, C., Vernazza, P., Villanueva, G. L.
The ice giants Uranus and Neptune are the least understood class of planets in our solar system but the most frequently observed type of exoplanets. Presumed to have a small rocky core, a deep interior comprising ~70% heavy elements surrounded by a m
Externí odkaz:
http://arxiv.org/abs/1708.00235
Context. The identification of the carriers of diffuse interstellar bands (DIBs) remains one of the long-standing mysteries in astronomy. The detection of a polarisation signal in a DIB profile can be used to distinguish between a dust or gas-phase c
Externí odkaz:
http://arxiv.org/abs/1104.4581
We present laboratory studies of the micro-structural evolution of an amorphous ferro-magnesian silicate, of olivine composition, following thermal annealing under vacuum. Annealing under vacuum was performed at temperatures ranging from 870 to 1020
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602079
Autor:
Thi, W. F., van Dishoeck, E. F., Dartois, E., Pontoppidan, K. M., Schutte, W. A., Ehrenfreund, P., d'Hendecourt, L., Fraser, H. J.
We performed a spectroscopic survey toward five intermediate-mass class I YSOs located in the Southern Vela molecular cloud in the L and M bands at resolving powers 600-800 up to 10,000, using the Infrared Spectrometer and Array Camera mounted on the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512186
Autor:
Mousis, O., Atkinson, D.H., Cavalié, T., Fletcher, L.N., Amato, M.J., Aslam, S., Ferri, F., Renard, J.-B., Spilker, T., Venkatapathy, E., Wurz, P., Aplin, K., Coustenis, A., Deleuil, M., Dobrijevic, M., Fouchet, T., Guillot, T., Hartogh, P., Hewagama, T., Hofstadter, M.D., Hue, V., Hueso, R., Lebreton, J.-P., Lellouch, E., Moses, J., Orton, G.S., Pearl, J.C., Sánchez-Lavega, A., Simon, A., Venot, O., Waite, J.H., Achterberg, R.K., Atreya, S., Billebaud, F., Blanc, M., Borget, F., Brugger, B., Charnoz, S., Chiavassa, T., Cottini, V., d'Hendecourt, L., Danger, G., Encrenaz, T., Gorius, N.J.P., Jorda, L., Marty, B., Moreno, R., Morse, A., Nixon, C., Reh, K., Ronnet, T., Schmider, F.-X., Sheridan, S., Sotin, C., Vernazza, P., Villanueva, G.L.
Publikováno v:
In Planetary and Space Science June 2018 155:12-40
Publikováno v:
Astron.Astrophys. 423 (2004) 549-558
We present ESO - Very Large Telescope and ESA - Infrared Space Observatory 3 to 4 $\mu$m spectra of Seyfert 2 nuclei as compared to our galactic center lines of sight. The diffuse interstellar medium probed in both environments displays the character
Externí odkaz:
http://arxiv.org/abs/astro-ph/0405327
Autor:
Pontoppidan, K. M., Fraser, H. J., Dartois, E., Thi, W. -F., van Dishoeck, E. F., Boogert, A. C. A., d'Hendecourt, L., Tielens, A. G. G. M., Bisschop, S. E.
Medium resolution (lambda/Delta lambda = 5000-10000) VLT-ISAAC M-band spectra are presented of 39 young stellar objects in nearby low-mass star forming clouds showing the 4.67 micron stretching vibration mode of solid CO. By taking advantage of the u
Externí odkaz:
http://arxiv.org/abs/astro-ph/0307097
Publikováno v:
Astron.Astrophys. 404 (2003) L17-L20
We present detections of the absorption band at 3.53 micron due to solid methanol toward three low-mass young stellar objects located in the Serpens and Chameleon molecular cloud complexes. The sources were observed as part of a large spectroscopic s
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304476