Zobrazeno 1 - 10
of 62
pro vyhledávání: '"V. Alí-Lagoa"'
Autor:
Vania Lorenzi, Humberto Campins, Zoe A. Landsman, Javier Licandro, Marco Delbo, V. Alí-Lagoa, Michael P. Lucas, Brian Burt, Francesca E. DeMeo, Kevin J. Walsh, J. de León, Noemi Pinilla-Alonso
Publikováno v:
Icarus. 274:231-248
The inner asteroid belt is an important source of near-Earth asteroids (NEAs). Dynamical studies of the inner asteroid belt have identified several families overlapping in proper orbital elements, including the Polana and Eulalia families that contai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a1a33016f8776bcf37fb72fdda1555d5
https://doi.org/10.1016/j.icarus.2016.03.022
https://doi.org/10.1016/j.icarus.2016.03.022
Autor:
Vania Lorenzi, V. Alí-Lagoa, Zoe A. Landsman, Alberto Cellino, P. Bendjoya, Francesca E. DeMeo, J. Gayon-Markt, Javier Licandro, David Morate, Marco Delbo, Kevin J. Walsh, Humberto Campins, J. de León, Antonio Cabrera-Lavers, Paolo Tanga, Noemi Pinilla-Alonso
Publikováno v:
Icarus. 266:57-75
The Polana-Eulalia family complex is located in the inner part of the asteroid belt, bounded by the ν6 and the 3:1 resonances, where we can find another three collisional families of primitive asteroids (Erigone, Clarissa, and Sulamitis), and a low-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7dfded418d2abeca31a9d332c276f9ae
https://doi.org/10.1016/j.icarus.2015.11.014
https://doi.org/10.1016/j.icarus.2015.11.014
Publikováno v:
Icarus. 256:101-116
In the analysis of thermal infrared data of asteroids by means of thermophysical models (TPMs) it is a common practice to neglect the uncertainty of the shape model and the rotational state, which are taken as an input for the model. Here, we present
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7456749d0151f0775c269a13a8f8990a
https://doi.org/10.1016/j.icarus.2015.04.014
https://doi.org/10.1016/j.icarus.2015.04.014
Autor:
V. Alí-Lagoa, Marco Delbo, Michael S. P. Kelley, Javier Licandro, M. Cañada-Assandri, Humberto Campins, J. de León, Ricardo Gil-Hutton, Josef Hanus, Noemi Pinilla-Alonso
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy & Astrophysics
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Astronomy & Astrophysics
Context. B-type asteroids constitute a peculiar spectral class within the C-complex. Previous work has pointed out the difference between the visible geometric albedos of B-types and those of the Pallas collisional family (PCF), whose few members wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::25db2078ca6a07775e075cf2ac615804
https://www.aanda.org/articles/aa/abs/2016/07/aa27660-15/aa27660-15.html
https://www.aanda.org/articles/aa/abs/2016/07/aa27660-15/aa27660-15.html
Autor:
Maxime Devogele, Leonard Kornoš, Josh Emery, Peter Kusnirak, Adrian Galad, Marco Delbo, V. Alí-Lagoa, Brian D. Warner, Javier Licandro, David Vokrouhlický, R. Dyvig, Robert Jedicke, Vishnu Reddy, J. P. Rivet, Josef Hanus, Petr Pravec, Jozef Vilagi, Bryce Bolin
The near-Earth asteroid (3200) Phaethon is an intriguing object: its perihelion is at only 0.14 au and is associated with the Geminid meteor stream. We aim to use all available disk-integrated optical data to derive a reliable convex shape model of P
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d5e4e484bfbee016a403395f495f5cd
The so-called "early activity" of comet 67P/Churyumov-Gerasimenko has been observed to originate mostly in parts of the concave region or "neck" between its two lobes. Since activity is driven by the sublimation of volatiles, this is a puzzling resul
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9d5ff4789eb725aa6c3e8a305bc42a4a
http://arxiv.org/abs/1509.03179
http://arxiv.org/abs/1509.03179
Autor:
Jean Manfroid, Marco Delbo, C. Vera Hernández, J. Lecacheux, Raoul Behrend, E. Frappa, Paolo Tanga, Julio Camargo, M. Audejean, Lucie Maquet, M. Conjat, Maxime Devogele, G. Dubos, M. Todd, Magdalena Polińska, N. Cornero, R. Roy, M. Cedrés Reyes, D. Coward, Marcelo Assafin, V. Alí Lagoa, A. Klotz, Hiromi Hamanowa, E. Morelle, F. Manzini, R. Crippa, Emmanuel Jehin, Frédéric Vachier, A. Matter, A. H. Andrei, A. Leroy, E. de Ferra Fantin, Albino Carbognani, P. Wiggins, Stefano Mottola, François Colas, Agnieszka Kryszczyńska, Michaël Gillon, Benoit Carry, Josef Hanus
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Monthly Notices of the Royal Astronomical Society, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Monthly Notices of the Royal Astronomical Society, 2015, 448 (4), pp.3382-3390. ⟨10.1093/mnras/stv229⟩
Asteroid (234) Barbara is the prototype of a category of asteroids that has been shown to be extremely rich in refractory inclusions, the oldest material ever found in the Solar System. It exhibits several peculiar features, most notably its polarime
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b61165d2d5178afbeb91eba76303dd2d
https://hal.archives-ouvertes.fr/hal-02483528
https://hal.archives-ouvertes.fr/hal-02483528
Autor:
Simon F. Green, Olivier Groussin, M. Reyes García-Talavera, Jörn Helbert, J. Le Merrer, Audrey Delsanti, Kjetil Dohlen, P. Lamy, E. Brageot, Jessica M. Sunshine, C. Rossin, J. Knollenberg, Ekkehard Kührt, Pierre Vernazza, V. Alí-Lagoa, P. Levacher, Ben Rozitis, Marco Delbo, J.-L. Reynaud, Didier Ferrand, Laurent Jorda, J. J. Díaz Garcia, Sébastien Vivès, Javier Licandro, Emmanuel Lellouch, P. E. Blanc, Bernard Marty, E. Joven Álvarez, M. Deleuze, Björn Davidsson, G. Mas
Publikováno v:
Experimental Astronomy
Experimental Astronomy, 2016, 41 (1), pp.95--115. ⟨10.1007/s10686-015-9475-9⟩
Experimental Astronomy, springer Link, 2016, 41 (1), pp.95--115. ⟨10.1007/s10686-015-9475-9⟩
Experimental Astronomy, 2016, 41 (1), pp.95--115. ⟨10.1007/s10686-015-9475-9⟩
Experimental Astronomy, springer Link, 2016, 41 (1), pp.95--115. ⟨10.1007/s10686-015-9475-9⟩
We present THERMAP, a mid-infrared (8-16 {\mu}m) spectro-imager for space missions to small bodies in the inner solar system, developed in the framework of the MarcoPolo-R asteroid sample return mission. THERMAP is very well suited to characterize th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0063380415c8cc710578c111efa59273
Autor:
P. Scheirich, David Polishook, Josef Ďurech, James W. Brinsfield, Seth A. Jacobson, Kamil Hornoch, Donald P. Pray, V. R. Ayvazian, Adrian Galad, Igor Molotov, Yu. N. Krugly, Michaël Gillon, I. Slyusarev, Petr Pravec, Joe Pollock, Michael Mommert, R. Ya. Inasaridze, J. Pittichová, Javier Licandro, Emmanuel Jehin, S. Hellmich, Jean Manfroid, V. Alí-Lagoa, Stefano Mottola, O. Kvaratskhelia, Peter Kusnirak
Using our photometric observations taken between 1996 and 2013 and other published data, we derived properties of the binary near-Earth asteroid (175706) 1996 FG3 including new measurements constraining evolution of the mutual orbit with potential co
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8911390c32b23c81a9db2dae0efc65ba
http://arxiv.org/abs/1406.4677
http://arxiv.org/abs/1406.4677
Publikováno v:
Astronomy & Astrophysics. 585:A10
Context. The potentially hazardous asteroid (PHA) (99942) Apophis is one of the most remarkable near-Earth asteroids (NEA) in terms of impact hazard. A good determination of its surface thermal inertia is very important in order to evaluate the Yarko
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8f81ffa0173e218ba39d71a66b17c535
https://doi.org/10.1051/0004-6361/201526888
https://doi.org/10.1051/0004-6361/201526888