Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Olga Harrington-Pinto"'
Publikováno v:
The Planetary Science Journal. 3:247
CO and CO2 are the two dominant carbon-bearing molecules in comae and have major roles in driving activity. Their relative abundances also provide strong observational constraints to models of solar system formation and evolution but have never been
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e1cadd5c5dc717a3f1139eb1ee448534
https://doi.org/10.3847/psj/ac960d
https://doi.org/10.3847/psj/ac960d
Autor:
Amy Mainzer, Yanga R. Fernandez, Jason Surace, Charles Schambeau, Tommy Grav, Eva Schunova, Olga Harrington-Pinto, Bonnie J. Buratti, Paul A. Abell, James M. Bauer, Emily Kramer, Neo Surveillance Mission Investigation Team
The Near-Earth Object Surveillance Mission (NEOSM) will provide unprecedented detection, tracking and characterization of Near-Earth Objects (NEOs) using high-cadence imaging from a space-based infrared telescope. Planning for the NEOSM requires an a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3eac84172257b0a9cceca5643649d68e
https://doi.org/10.5194/epsc2020-460
https://doi.org/10.5194/epsc2020-460
Autor:
Joseph L. Hora, Olga Harrington Pinto, Jessica Agarwal, Maria Womack, Michael S. P. Kelley, David Trilling, Howard A. Smith, N. Moskovitz, David Polishook, Kacper Wierzchos, Michael Mommert, Nicolas Biver, Matthew M. Knight, Andrew McNeill, Yoonyoung Kim
Publikováno v:
The Planetary Science Journal
The Planetary Science Journal, IOP Science, 2020, 1 (1), pp.12. ⟨10.3847/PSJ/ab8ae5⟩
The Planetary Science Journal, IOP Science, 2020, 1 (1), pp.12. ⟨10.3847/PSJ/ab8ae5⟩
We report on observations of activity in near-Earth object (3552) Don Quixote using the Spitzer Space Telescope and ground-based telescopes around its 2018 perihelion passage. Spitzer observations obtained six months before perihelion show extended e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c842364c34db3b5c12a8b459de04f6b4
https://doi.org/10.3847/psj/ab8ae5
https://doi.org/10.3847/psj/ab8ae5
Autor:
James M. Bauer, Maria Womack, Nicolas Biver, Michael A. DiSanti, Michael S. P. Kelley, Anita L. Cochran, Erika L. Gibb, Nathan Roth, Ronald J. Vervack, Kacper Wierzchos, Adam J. McKay, Olga Harrington Pinto, Hideyo Kawakita, Neil Dello Russo, Matthew M. Knight, Geronimo L. Villanueva, Boncho P. Bonev
Publikováno v:
The Astronomical Journal
The Astronomical Journal, American Astronomical Society, 2019, 158 (3), pp.128. ⟨10.3847/1538-3881/ab32e4⟩
The Astronomical Journal, American Astronomical Society, 2019, 158 (3), pp.128. ⟨10.3847/1538-3881/ab32e4⟩
Comet C/2016 R2 (PanSTARRS) has a peculiar volatile composition, with CO being the dominant volatile as opposed to H$_2$O and one of the largest N$_2$/CO ratios ever observed in a comet. Using observations obtained with the \textit{Spitzer Space Tele
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c389361cccd79d43dbf4fabb9cdbb607
https://doi.org/10.3847/1538-3881/ab32e4
https://doi.org/10.3847/1538-3881/ab32e4
Autor:
Adam J. McKay, Michael A. DiSanti, Michael S. P. Kelley, Matthew M. Knight, Maria Womack, Kacper Wierzchos, Olga Harrington Pinto, Boncho Bonev, Geronimo L. Villanueva, Neil Dello Russo, Anita L. Cochran, Nicolas Biver, James Bauer, Ronald J. Vervack, Jr., Erika Gibb, Nathan Roth, Hideyo Kawakita
Publikováno v:
Astronomical Journal; Sep2019, Vol. 158 Issue 3, p1-1, 1p