Zobrazeno 1 - 10
of 56
pro vyhledávání: '"planetary systems [Infrared]"'
Infrared measurements of asteroids are crucial for the determination of physical and thermal properties of individual objects, and for the understanding of the small-body populations in the solar system as a whole. But standard radiometric methods ca
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::33369a78e865813746f33b901baa2e18
http://arxiv.org/abs/2302.06921
http://arxiv.org/abs/2302.06921
Autor:
Bockelée-Morvan, D., Biver, N., Schambeau, C. A., Crovisier, J., Opitom, C., Borro, M. de Val, Lellouch, E., Hartogh, P., Vandenbussche, B., Jehin, E., Kidger, M., Küppers, M., Lis, D. C., Moreno, R., Szutowicz, S., Zakharov, V.
Publikováno v:
Astronomy and Astrophysics
Bockelée-Morvan, D, Biver, N, Schambeau, C A, Crovisier, J, Opitom, C, Borro, M D V, Lellouch, E, Hartogh, P, Vandenbussche, B, Jehin, E, Kidger, M, Küppers, M, Lis, D C, Moreno, R, Szutowicz, S & Zakharov, V 2022, ' Water, hydrogen cyanide, carbon monoxide, and dust production from distant comet 29P/Schwassmann-Wachmann 1 ', Astronomy and Astrophysics, vol. 664, A95, pp. 1-27 . https://doi.org/10.1051/0004-6361/202243241
Bockelée-Morvan, D, Biver, N, Schambeau, C A, Crovisier, J, Opitom, C, Borro, M D V, Lellouch, E, Hartogh, P, Vandenbussche, B, Jehin, E, Kidger, M, Küppers, M, Lis, D C, Moreno, R, Szutowicz, S & Zakharov, V 2022, ' Water, hydrogen cyanide, carbon monoxide, and dust production from distant comet 29P/Schwassmann-Wachmann 1 ', Astronomy and Astrophysics, vol. 664, A95, pp. 1-27 . https://doi.org/10.1051/0004-6361/202243241
29P/Schwassmann-Wachmann 1 is a distant Centaur/comet, showing persistent CO-driven activity and frequent outbursts. We used the Herschel space observatory in 2010, 2011, and 2013 to observe H$_2$O and NH$_3$ and to image the dust coma. Observations
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b83ed6be3503164d5da28b165ed40b8e
Autor:
Quanz, S. P., Ottiger, M., Fontanet, E., Kammerer, J., Menti, F., Dannert, F., Gheorghe, A., Absil, O., Airapetian, V. S., Alei, E., Allart, R., Angerhausen, D., Blumenthal, S., Buchhave, L. A., Cabrera, J., Carrión-González, Ó., Chauvin, G., Danchi, W. C., Dandumont, C., Defrére, D., Dorn, C., Ehrenreich, D., Ertel, S., Fridlund, M., García Muñoz, A., Gascón, C., Girard, J. H., Glauser, A., Grenfell, J. L., Guidi, G., Hagelberg, J., Helled, R., Ireland, M. J., Janson, M., Kopparapu, R. K., Korth, J., Kozakis, T., Kraus, S., Léger, A., Leedjärv, L., Lichtenberg, T., Lillo-Box, J., Linz, H., Liseau, R., Loicq, J., Mahendra, V., Malbet, F., Mathew, J., Mennesson, B., Meyer, M. R., Mishra, L., Molaverdikhani, K., Noack, L., Oza, A. V., Pallé, E., Parviainen, H., Quirrenbach, A., Rauer, H., Ribas, I., Rice, M., Romagnolo, A., Rugheimer, S., Schwieterman, E. W., Serabyn, E., Sharma, S., Stassun, K. G., Szulágyi, J., Wang, H. S., Wunderlich, F., Wyatt, M. C., Collaboration, the LIFE
Publikováno v:
Quanz, S P, Ottiger, M, Fontanet, E, Kammerer, J, Menti, F, Dannert, F, Gheorghe, A, Absil, O, Airapetian, V S, Alei, E, Allart, R, Angerhausen, D, Blumenthal, S, Buchhave, L A, Cabrera, J, Carrión-González, Ó, Chauvin, G, Danchi, W C, Dandumont, C, Defrére, D, Dorn, C, Ehrenreich, D, Ertel, S, Fridlund, M, García Muñoz, A, Gascón, C, Girard, J H, Glauser, A, Grenfell, J L, Guidi, G, Hagelberg, J, Helled, R, Ireland, M J, Janson, M, Kopparapu, R K, Korth, J, Kozakis, T, Kraus, S, Léger, A, Leedjärv, L, Lichtenberg, T, Lillo-Box, J, Linz, H, Liseau, R, Loicq, J, Mahendra, V, Malbet, F, Mathew, J, Mennesson, B, Meyer, M R, Mishra, L, Molaverdikhani, K, Noack, L, Oza, A V, Pallé, E, Parviainen, H, Quirrenbach, A, Rauer, H, Ribas, I, Rice, M, Romagnolo, A, Rugheimer, S, Schwieterman, E W, Serabyn, E, Sharma, S, Stassun, K G, Szulágyi, J, Wang, H S, Wunderlich, F, Wyatt, M C & Collaboration, T LIFE 2022, ' Large Interferometer For Exoplanets (LIFE) ', Astronomy and Astrophysics, vol. 664, A21 . https://doi.org/10.1051/0004-6361/202140366
Context. One of the long-term goals of exoplanet science is the atmospheric characterization of dozens of small exoplanets in order to understand their diversity and search for habitable worlds and potential biosignatures. Achieving this goal require
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od______1202::97ae27b4363b62546edcbc55e7a06576
https://orbit.dtu.dk/en/publications/99e7cc47-6f91-4ad4-b2b2-df8e8229210e
https://orbit.dtu.dk/en/publications/99e7cc47-6f91-4ad4-b2b2-df8e8229210e
Autor:
Michiel Min, Mark W. Phillips, Ingo Waldmann, Ahmed Al-Refaie, Katy L. Chubb, Jonathan Tennyson, Paul Mollière, Marco Rocchetto, Sergei N. Yurchenko, Joanna K. Barstow
Publikováno v:
Astronomy & Astrophysics
A publicly available database of opacities for molecules of astrophysical interest, ExoMolOP, has been compiled for over 80 species, based on the latest line list data from the ExoMol, HITEMP and MoLLIST databases. These data are generally suitable f
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb412182c8ed29273f7e56dd883c82e4
https://hdl.handle.net/10023/24479
https://hdl.handle.net/10023/24479
Autor:
Manuel López-Puertas, M. R. Zapatero Osorio, Lev Tal-Or, Mathias Zechmeister, Enric Palle, Víctor J. S. Béjar, Karan Molaverdikhani, Th. Henning, Lisa Nortmann, Andreas Quirrenbach, S. Czesla, J. Aceituno, P. J. Amado, Ansgar Reiners, F. F. Bauer, A. Sánchez-López, M. Stangret, J. A. Caballero, Ignas Snellen, Núria Casasayas-Barris, Evangelos Nagel, D. Montes, Ignasi Ribas
Publikováno v:
Astronomy & Astrophysics, 643, A24
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Digital.CSIC. Repositorio Institucional del CSIC
instname
E-Prints Complutense. Archivo Institucional de la UCM
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
Instituto Nacional de Técnica Aeroespacial (INTA)
Astronomy & Astrophysics
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Context. Relatively large radii of some hot Jupiters observed in the ultraviolet and blue-optical are generally interpreted to be due to Rayleigh scattering by high-altitude haze particles. However, the haze composition and its production mechanisms
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c116ad21d2952bf1e94583b5fb155e8
http://hdl.handle.net/1887/3133910
http://hdl.handle.net/1887/3133910
Autor:
Encrenaz, Thérèse, Greathouse, Thomas K., Marcq, Emmanuel, Sagawa, H., Widemann, Thomas, Bézard, Bruno, Fouchet, Thierry, Lefèvre, Franck, Lebonnois, Sébastien, Atreya, S. K., Lee, Y. J., Giles, R., Watanabe, S., Shao, W., Zhang, Xi, Bierson, C. J.
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 639, pp.A69. ⟨10.1051/0004-6361/202037741⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A69. ⟨10.1051/0004-6361/202037741⟩
Astronomy and Astrophysics-A&A, 2020, 639, pp.A69. ⟨10.1051/0004-6361/202037741⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 639, pp.A69. ⟨10.1051/0004-6361/202037741⟩
International audience Since January 2012, we have been monitoring the behavior of sulfur dioxide and water on Venus, using the Texas Echelon Cross-Echelle Spectrograph imaging spectrometer at the NASA InfraRed Telescope Facility (IRTF, Mauna Kea Obs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::b442a8fbb70c13a8292566deba559b10
https://hal-insu.archives-ouvertes.fr/insu-02637956/document
https://hal-insu.archives-ouvertes.fr/insu-02637956/document
Autor:
M. Butkiewicz-Bąk, Róbert Szakáts, Przemyslaw Bartczak, Victor Ali-Lagoa, Anna Marciniak, A. Farkas-Takács, Gábor Marton, Pablo Santos-Sanz, Grzegorz Dudziński, Rene Duffard, T. G. Müller, Cs. Kiss, E. Podlewska-Gaca, Jose Luis Ortiz
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the origi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7d562f0d3e50aa889a7e1cc1ff3ea9dc
Publikováno v:
Astronomy & Astrophysics
We have conducted a re-analysis of publicly available Hubble Space Telescope Wide Field Camera 3 (HST WFC3) transmission data for the hot-Jupiter exoplanet WASP-43b, using the Bayesian retrieval package Tau-REx. We report evidence of AlO in transmiss
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::78ff303654d69faa6dcf4e5e88494b18
Autor:
Athena Coustenis, Donald E. Jennings, Nicholas A. Lombardo, Nicholas A Teanby, Conor A. Nixon, Gordon L. Bjoraker, Regis Courtin, Paul N. Romani, Carrie M. Anderson, F. Michael Flasar, Bruno Bézard, Sandrine Vinatier, Valeria Cottini, Robert E. Samuelson, Todd M. Ansty, Richard Achterberg, A. M. Annex, Emmanuel Lellouch, Malena Rice
Publikováno v:
Astrophysical Journal Supplement
Astrophysical Journal Supplement, American Astronomical Society, 2019, 244 (1), pp.14. ⟨10.3847/1538-4365/ab3799⟩
Nixon, CA, Teanby, N & al, E 2019, ' Cassini Composite Infrared Spectrometer (CIRS) Observations of Titan 2004–2017 ', Astrophysical Journal Supplement Series, vol. 244, no. 1 . https://doi.org/10.3847/1538-4365/ab3799
Astrophysical Journal Supplement, American Astronomical Society, 2019, 244 (1), pp.14. ⟨10.3847/1538-4365/ab3799⟩
Nixon, CA, Teanby, N & al, E 2019, ' Cassini Composite Infrared Spectrometer (CIRS) Observations of Titan 2004–2017 ', Astrophysical Journal Supplement Series, vol. 244, no. 1 . https://doi.org/10.3847/1538-4365/ab3799
From 2004 to 2017, the Cassini spacecraft orbited Saturn, completing 127 close flybys of its largest moon, Titan. Cassini's Composite Infrared Spectrometer (CIRS), one of 12 instruments carried on board, profiled Titan in the thermal infrared (7-1000
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83e59beb90949d9c49c5944033d79bda
https://hal.archives-ouvertes.fr/hal-02329695
https://hal.archives-ouvertes.fr/hal-02329695
Autor:
Johan Olofsson, Renu Malhotra, Keivan G. Stassun, D. E. Reichart, Kate Y. L. Su, Ruobing Dong, Wiphu Rujopakarn, Joseph E. Rodriguez, Alan Jackson, George H. Rieke, Joshua Pepper, David James, Zoë M. Leinhardt, Grant M. Kennedy, Huan Meng, Michael Hammer, Andras Gaspar
Publikováno v:
Su, K Y L, Jackson, A P, Gáspár, A, Rieke, G H, Dong, R, Olofsson, J, Kennedy, G M, Leinhardt, Z M, Malhotra, R, Hammer, M, Meng, H Y A, Rujopakarn, W, Rodriguez, J E, Pepper, J, Reichart, D E, James, D & Stassun, K G 2019, ' Extreme Debris Disk Variability : Exploring the Diverse Outcomes of Large Asteroid Impacts during the Era of Terrestrial Planet Formation ', Astronomical Journal, vol. 157, no. 5 . https://doi.org/10.3847/1538-3881/ab1260
The most dramatic phases of terrestrial planet formation are thought to be oligarchic and chaotic growth, on timescales of up to 100-200 Myr, when violent impacts occur between large planetesimals of sizes up to proto-planets. Such events are marked
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d8603a93cbdd38b1b5fbcbbd031c369
http://wrap.warwick.ac.uk/116936/7/WRAP-extreme-debris-disk-variability-exploring-diverse-outcomes-large-asteroid-Grant-2019.pdf
http://wrap.warwick.ac.uk/116936/7/WRAP-extreme-debris-disk-variability-exploring-diverse-outcomes-large-asteroid-Grant-2019.pdf