Zobrazeno 1 - 10
of 178
pro vyhledávání: '"Kolokolova Ludmilla"'
Autor:
Kwon, Yuna G., Bagnulo, Stefano, Markkanen, Johannes, Kolokolova, Ludmilla, Agarwal, Jessica, Lippi, Manuela, Gray, Zuri
Comets, relics from the early solar system, consist of dust and ice. The ice sublimates as comets approach the Sun, ejecting dust from their nuclei seen as activity. Different volatiles sublimate at different Sun-comet distances and eject dust of uni
Externí odkaz:
http://arxiv.org/abs/2408.01636
Autor:
Gray, Zuri, Bagnulo, Stefano, Boehnhardt, Hermann, Borisov, Galin, Jones, Geraint H., Kolokolova, Ludmilla, Kwon, Yuna G., Moreno, Fernando, Muñoz, Olga, Nežič, Rok, Snodgrass, Colin
Comet 67P/Churyumov-Gerasimenko (67P) become observable for the first time in 2021 since the Rosetta rendezvous in 2014--16. Here, we present pre-perihelion polarimetric measurements of 67P from 2021 performed with the Very Large Telescope (VLT), as
Externí odkaz:
http://arxiv.org/abs/2405.09297
Autor:
Hom, Justin, Patience, Jennifer, Chen, Christine H., Duchêne, Gaspard, Mazoyer, Johan, Millar-Blanchaer, Maxwell A., Esposito, Thomas M., Kalas, Paul, Crotts, Katie A., Gonzales, Eileen C., Kolokolova, Ludmilla, Lewis, Briley L., Matthews, Brenda C., Rice, Malena, Weinberger, Alycia J., Wilner, David J., Wolff, Schuyler G., Bruzzone, Sebastián, Choquet, Elodie, Debes, John, De Rosa, Robert J., Donaldson, Jessica, Draper, Zachary, Fitzgerald, Michael P., Hines, Dean C., Hinkley, Sasha, Hughes, A. Meredith, López, Ronald A., Marchis, Franck, Metchev, Stanimir, Moro-Martin, Amaya, Nesvold, Erika, Nielsen, Eric L., Oppenheimer, Rebecca, Padgett, Deborah, Perrin, Marshall D., Pueyo, Laurent, Rantakyrö, Frederik, Ren, Bin B., Schneider, Glenn, Soummer, Remí, Song, Inseok, Stark, Christopher C.
Spatially-resolved images of debris disks are necessary to determine disk morphological properties and the scattering phase function (SPF) which quantifies the brightness of scattered light as a function of phase angle. Current high-contrast imaging
Externí odkaz:
http://arxiv.org/abs/2402.00214
Autor:
Crotts, Katie A., Matthews, Brenda C., Duchêne, Gaspard, Esposito, Thomas M., Dong, Ruobing, Hom, Justin, Oppenheimer, Rebecca, Rice, Malena, Wolff, Schuyler G., Chen, Christine H., Ó, Clarissa R. Do, Kalas, Paul, Lewis, Briley L., Weinberger, Alycia J., Wilner, David J., Ammons, Mark, Arriaga, Pauline, De Rosa, Robert J., Debes, John H., Fitzgerald, Michael P., Gonzales, Eileen C., Hines, Dean C., Hinkley, Sasha, Hughes, A. Meredith, Kolokolova, Ludmilla, Lee, Eve J., López, Ronald A., Macintosh, Bruce, Mazoyer, Johan, Metchev, Stanimir, Millar-Blanchaer, Maxwell A., Nielsen, Eric L., Patience, Jenny, Perrin, Marshall D., Pueyo, Laurent, Rantakyrö, Fredrik T., Ren, Bin B., Schneider, Glenn, Soummer, Remi, Stark, Christopher C.
The Gemini Planet Imager (GPI) has excelled in imaging debris disks in the near-infrared. The GPI Exoplanet Survey (GPIES) imaged twenty-four debris disks in polarized $H$-band light, while other programs observed half of these disks in polarized $J$
Externí odkaz:
http://arxiv.org/abs/2311.14599
Autor:
Gray, Zuri, Bagnulo, Stefano, Granvik, Mikael, Cellino, Alberto, Jones, Geraint H., Kolokolova, Ludmilla, Moreno, Fernando, Muinonen, Karri, Muñoz, Olga, Opitom, Cyrielle, Penttilä, Antti, Snodgrass, Colin
We have monitored the Didymos-Dimorphos binary system in imaging polarimetric mode before and after the impact from the Double Asteroid Redirection Test (DART) mission. A previous spectropolarimetric study showed that the impact caused a dramatic dro
Externí odkaz:
http://arxiv.org/abs/2311.13483
Autor:
Moreno, Fernando, Bagatin, Adriano Campo, Tancredi, Gonzalo, Li, Jian-Yang, Rossi, Alessandro, Ferrari, Fabio, Hirabayashi, Masatoshi, Fahnestock, Eugene, Maury, Alain, Sandness, Robert, Rivkin, Andrew S., Cheng, Andy, Farnham, Tony L., Soldini, Stefania, Giordano, Carmine, Merisio, Gianmario, Panicucci, Paolo, Pugliatti, Mattia, Castro-Tirado, Alberto J., Fernandez-Garcia, Emilio, Perez-Garcia, Ignacio, Ivanovski, Stavro, Penttila, Antti, Kolokolova, Ludmilla, Licandro, Javier, Munoz, Olga, Gray, Zuri, Ortiz, Jose L., Lin, Zhong-Yi
The NASA/DART (Double Asteroid Redirection Test) spacecraft successfully crashed on Dimorphos, the secondary component of the binary (65803) Didymos system. Following the impact, a large dust cloud was released, and a long-lasting dust tail was devel
Externí odkaz:
http://arxiv.org/abs/2307.10086
Autor:
Li, Jian-Yang, Hirabayashi, Masatoshi, Farnham, Tony L., Sunshine, Jessica M., Knight, Matthew M., Tancredi, Gonzalo, Moreno, Fernando, Murphy, Brian, Opitom, Cyrielle, Chesley, Steve, Scheeres, Daniel J., Thomas, Cristina A., Fahnestock, Eugene G., Cheng, Andrew F., Dressel, Linda, Ernst, Carolyn M., Ferrari, Fabio, Fitzsimmons, Alan, Ieva, Simone, Ivanovski, Stavro L., Kareta, Teddy, Kolokolova, Ludmilla, Lister, Tim, Raducan, Sabina D., Rivkin, Andrew S., Rossi, Alessandro, Soldini, Stefania, Stickle, Angela M., Vick, Alison, Vincent, Jean-Baptiste, Weaver, Harold A., Bagnulo, Stefano, Bannister, Michele T., Cambioni, Saverio, Bagatin, Adriano Campo, Chabot, Nancy L., Cremonese, Gabriele, Daly, R. Terik, Dotto, Elisabetta, Glenar, David A., Granvik, Mikael, Hasselmann, Pedro H., Herreros, Isabel, Jacobson, Seth, Jutzi, Martin, Kohout, Tomas, La Forgia, Fiorangela, Lazzarin, Monica, Lin, Zhong-Yi, Lolachi, Ramin, Lucchetti, Alice, Makadia, Rahil, Epifani, Elena Mazzotta, Michel, Patrick, Migliorini, Alessandra, Moskovitz, Nicholas A., Orm., Jens, Pajola, Maurizio, nchez, Paul S., Schwartz, Stephen R., Snodgrass, Colin, Steckloff, Jordan, Stubbs, Timothy J., Trigo-Rodriguez, Josep M.
Some active asteroids have been proposed to be the result of impact events. Because active asteroids are generally discovered serendipitously only after their tail formation, the process of the impact ejecta evolving into a tail has never been direct
Externí odkaz:
http://arxiv.org/abs/2303.01700
Publikováno v:
Planet.Sci.J. 3 (2022) 135
C/2017 K2 (PANSTARRS) is an Oort cloud comet previously observed to be active at heliocentric distances r>20 au on what is likely its first passage through the inner solar system. We observed the comet on 2021 March 19-20 at r=6.82 au pre-perihelion
Externí odkaz:
http://arxiv.org/abs/2205.02854
Autor:
Kimura, Hiroshi, Markkanen, Johannes, Kolokolova, Ludmilla, Hilchenbach, Martin, Wada, Koji, Kanada, Yasumasa, Matsui, Takafumi
A well-established constraint on the size of non-porous olivine grains or the porosity of aggregates consisting of small olivine grains from prominent narrow peaks in thermal infrared spectra characteristic of crystalline silicates is reexamined. To
Externí odkaz:
http://arxiv.org/abs/2203.04529