Zobrazeno 1 - 10
of 72
pro vyhledávání: '"general [asteroids]"'
Autor:
C. Opitom, B. Murphy, C. Snodgrass, S. Bagnulo, S. F. Green, M. M. Knight, J. de Léon, J.-Y. Li, D. Gardener
Publikováno v:
Opitom, C, Murphy, B, Snodgrass, C, Bagnulo, S, Green, S F, Knight, M M, de Leon, J, Li, J-Y & Gardener, D 2023, ' Morphology and spectral properties of the DART impact ejecta with VLT/MUSE ', Astronomy and Astrophysics, vol. 671, L11, pp. 1-7 . https://doi.org/10.1051/0004-6361/202345960
Context. On September 26, 2022, the NASA DART mission impacted the asteroid Dimorphos, the smaller component of the Didymos binary asteroid system. This provided a unique opportunity to observe, in real time, the evolution of the ejecta cloud produce
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f6e54fd0ee087cb3d6ef5968b559811e
https://hdl.handle.net/20.500.11820/d022be6d-6a0c-48c1-ac4a-3b32e4799ee1
https://hdl.handle.net/20.500.11820/d022be6d-6a0c-48c1-ac4a-3b32e4799ee1
Autor:
A. Malgoyre, Mar Tapia, D. Rousseu, C. Davadan, S. Jeanne, Detlef Koschny, Theresa Ott, Cyril Blanpain, D. A. Nedelcu, J. Lecubin, Pierre Vernazza, P. Cauhape, Esther Drolshagen, J. Vaubaillon, Brigitte Zanda, Agustín Sánchez-Lavega, Josep M. Trigo-Rodríguez, Mirel Birlan, J. L. Rault, S. Anghel, P. Dupouy, E. Peña-Asensio, M. Herpin, S. J. Ribas, Laurent Jorda, Jérôme Gattacceca, Ricardo Hueso, B. Tregon, Albert Rimola, François Colas, Sylvain Bouley
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Anghel, S., et al.
The increase in detector sensitivity and availability in the past three decades has allowed us to derive knowledge of the meteoroid flux and impact energy into the Earth's atmosphere. We present the multi-instrument detected 2
The increase in detector sensitivity and availability in the past three decades has allowed us to derive knowledge of the meteoroid flux and impact energy into the Earth's atmosphere. We present the multi-instrument detected 2
Publikováno v:
Digital.CSIC: Repositorio Institucional del CSIC
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Consejo Superior de Investigaciones Científicas (CSIC)
Digital.CSIC. Repositorio Institucional del CSIC
instname
The Gaia mission will provide the scientific community with high-quality observations of asteroids of all categories. The second release of Gaia data (DR2) was published in 2018 and consists of 22 months of observations of 14 099 known Solar system o
Autor:
Teymoor Saifollahi, Gijs Verdoes Kleijn, Rees Williams, Marco Micheli, Toni Santana-Ros, Ewout Helmich, Detlef Koschny, Luca Conversi
Publikováno v:
Astronomy & Astrophysics. 673:A93
Increasing our knowledge of the orbits and compositions of Near-Earth Objects (NEOs) is important for a better understanding of the evolution of the Solar System and of life. The detection of serendipitous NEO appearances among the millions of archiv
The first proposed Brazilian mission to deep space, the ASTER mission, has the triple asteroid system (153591) 2001 SN263 as a target. One of the mission's main goals is to analyze the physical and dynamical structures of the system to understand its
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b844a881ec3f485f68bddad3bf533e28
Publikováno v:
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
COLIBRI
Universidad de la República
instacron:Universidad de la República
Universidad de Alicante (UA)
COLIBRI
Universidad de la República
instacron:Universidad de la República
This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted reuse, distribution, and reproduction in any medium, provided the origin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::47548b63e856a2a7f381328d12996903
http://hdl.handle.net/10045/126125
http://hdl.handle.net/10045/126125
Autor:
J. Krajewski, P. Aurard, Philippe Lamy, Vishnu Reddy, Laurent Jorda, D. Molina, Josef Hanus, Josef Ďurech, P. Michel, F. Vachier, Nicolas Rambaux, J. Oey, Grzegorz Dudziński, P. Bartczak, A. Leroy, Michael Marsset, L. Dalmon, P. Beck, H. Le Coroller, Hiroko Hamanowa, Maëlle Neveu, Christophe Dumas, Hiromi Hamanowa, A. G. Sanchez, Zouhair Benkhaldoun, N. Payre, E. Podlewska-Gaca, Fabrice Cipriani, Raoul Behrend, Paolo Tanga, Aled Jones, Julie Castillo-Rogez, Miroslav Brož, P. Antonini, Tadeusz Michalowski, F. Livet, O. Labrevoir, J. M. Bosch, Emmanuel Jehin, Arthur Vigan, S. Fauvaud, A. Chapman, Marin Ferrais, Jérôme Berthier, Alexis Drouard, Mirel Birlan, J. Grice, R. Montaigut, J. His, L. Socha, Romain Fétick, Olivier Witasse, Pierre Vernazza, Thierry Fusco, Benoit Carry, F. Marchis, Doeon Kim, Toni Santana-Ros, Mikko Kaasalainen, Matti Viikinkoski, P. Sabin, M. Audejean, A. Marciniak, Myung-Jin Kim, Bin Yang, Agnieszka Kryszczyńska, François Colas
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A56. ⟨10.1051/0004-6361/202141781⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, 2021, 654, pp.A56. ⟨10.1051/0004-6361/202141781⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A56. ⟨10.1051/0004-6361/202141781⟩
RUA. Repositorio Institucional de la Universidad de Alicante
Universidad de Alicante (UA)
Astronomy and Astrophysics-A&A, 2021, 654, pp.A56. ⟨10.1051/0004-6361/202141781⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Vernazza, P., et al.
Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remai
Until recently, the 3D shape, and therefore density (when combining the volume estimate with available mass estimates), and surface topography of the vast majority of the largest (D ≥ 100 km) main-belt asteroids have remai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a582d603789efa8c1fec089600157a07
https://hal.archives-ouvertes.fr/hal-03375585/document
https://hal.archives-ouvertes.fr/hal-03375585/document
Autor:
Björn Poppe, B. Zanda, C. A. Volpicelli, J. Vaubaillon, Jim Rowe, Detlef Koschny, Pierre Vernazza, O. Hernandez, François Colas, Dan Alin Nedelcu, M. Forcier, Sylvain Bouley, Theresa Ott, Agustín Sánchez-Lavega, Josep M. Trigo-Rodríguez, Cristina Knapic, S. Rasetti, Esther Drolshagen, Daniele Gardiol, A. Toni, M. Di Carlo, Giovanni Pratesi, H. Lamy, Giovanni B. Valsecchi, Ludovic Ferrière, Sonia Zorba, E. Peña-Asensio, Mirel Birlan, Albert Rimola, A. Malgoyre, M. Jobin, S. Jeanne, Ashley J. King, Albino Carbognani, Emmanuel Jehin, Dario Barghini, Gerhard Drolshagen, W. Riva, G. M. Stirpe, A. Grandchamps, M. Di Martino
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A159. ⟨10.1051/0004-6361/202040204⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2021, 650, pp.A159. ⟨10.1051/0004-6361/202040204⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 650, pp.A159. ⟨10.1051/0004-6361/202040204⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A, 2021, 650, pp.A159. ⟨10.1051/0004-6361/202040204⟩
Drolshagen, E., et al.
[Context] In meteor physics, the luminous efficiency τ is used to convert the meteor's magnitude to the corresponding meteoroid's mass. However, a lack of sufficiently accurate verification methods or adequate laboratory
[Context] In meteor physics, the luminous efficiency τ is used to convert the meteor's magnitude to the corresponding meteoroid's mass. However, a lack of sufficiently accurate verification methods or adequate laboratory
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11886e4e47f778a1994f43295fb47166
https://hal.archives-ouvertes.fr/hal-03407196
https://hal.archives-ouvertes.fr/hal-03407196
Publikováno v:
Scopus
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Repositório Institucional da UNESP
Universidade Estadual Paulista (UNESP)
instacron:UNESP
Made available in DSpace on 2021-06-25T11:16:16Z (GMT). No. of bitstreams: 0 Previous issue date: 2021-06-01 Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) Coor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f5449271bec6c1e48336d30504b9385
Autor:
Javier Licandro, Renato A. Dupke, Jailson S. Alcaniz, Mariano Moles, Mário De Prá, C. Hernández-Monteagudo, Jorge Márcio Carvano, Antonio Marín-Franch, Jesús A. Varela, Javier Cenarro, Carlos López-Sanjuan, Alvaro Alvarez-Candal, David Morate, Raul E. Angulo, Héctor Vázquez Ramió, Beatriz B. Siffert, A. Galarza, Laerte Sodré, A. Ederoclite, Enrique Solano-Márquez, F. M. Jiménez-Esteban, David Cristóbal-Hornillos, Max Mahlke
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Context. The Javalambre Photometric Local Universe Survey (J-PLUS) is an observational campaign that aims to obtain photometry in 12 ultraviolet-visible filters (0.3-1 μm) over ∼8500 deg2 of the sky observable from Javalambre (Teruel, Spain). Due
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::931d837561e066c19920a5a7ea494238