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pro vyhledávání: '"Rockcliffe, Keighley"'
Autor:
Morrissey, Ava, Zhou, George, Huang, Chelsea X., Wright, Duncan, Auger, Caitlin, Rockcliffe, Keighley E., Newton, Elisabeth R., Rogers, James G., Gibson, Neale, Lowson, Nataliea, Mayorga, Laura C., Wittenmyer, Robert A.
HIP94235 b, a 120 Myr old sub-Neptune, provides us the unique opportunity to study mass loss at a pivotal stage of the system's evolution: the end of a 100 million year (Myr) old phase of intense XUV irradiation. We present two observations of HIP942
Externí odkaz:
http://arxiv.org/abs/2408.02170
Autor:
Rockcliffe, Keighley E., Newton, Elisabeth R., Youngblood, Allison, Duvvuri, Girish M., Plavchan, Peter, Gao, Peter, Mann, Andrew W., Lowrance, Patrick J.
Publikováno v:
The Astronomical Journal, Volume 166, Number 2, 2023
Photoevaporation is a potential explanation for several features within exoplanet demographics. Atmospheric escape observed in young Neptune-sized exoplanets can provide insight into and characterize which mechanisms drive this evolution and at what
Externí odkaz:
http://arxiv.org/abs/2307.15024
Autor:
Flagg, Laura, Johns-Krull, Christopher, France, Kevin, Herczeg, Gregory, Najita, Joan, Youngblood, Allison, Carvalho, Adolfo, Carptenter, John, Kenyon, Scott J., Newton, Elisabeth R., Rockcliffe, Keighley
Molecular hydrogen is the most abundant molecule in the Galaxy and plays important roles for planets, their circumstellar environments, and many of their host stars. We have confirmed the presence of molecular hydrogen in the AU Mic system using high
Externí odkaz:
http://arxiv.org/abs/2206.02636
Autor:
Rockcliffe, Keighley E., Newton, Elisabeth R., Youngblood, Allison, Bourrier, Vincent, Mann, Andrew W., Berta-Thompson, Zachory, Agüeros, Marcel A., Núñez, Alejandro, Charbonneau, David
Publikováno v:
AJ, 162, 116 (2021)
K2-25b is a Neptune-sized exoplanet (3.45 Earth radii) that orbits its M4.5 host with a period of 3.48 days. Due to its membership in the Hyades Cluster, the system has a known age (727 +/- 75 Myr). K2-25b's youth and its similarities with Gl 436b su
Externí odkaz:
http://arxiv.org/abs/2109.04376
Autor:
Mann, Andrew W., Johnson, Marshall C., Vanderburg, Andrew, Kraus, Adam L., Rizzuto, Aaron C., Wood, Mackenna L., Bush, Jonathan L., Rockcliffe, Keighley, Newton, Elisabeth R., Latham, David W., Mamajek, Eric E., Zhou, George, Quinn, Samuel N., Thao, Pa Chia, Benatti, Serena, Cosentino, Rosario, Desidera, Silvano, Harutyunyan, Avet, Lovis, Christophe, Mortier, Annelies, Pepe, Francesco A., Poretti, Ennio, Wilson, Thomas G., Kristiansen, Martti H., Gagliano, Robert, Jacobs, Thomas, LaCourse, Daryll M., Omohundro, Mark, Schwengeler, Hans Martin, Terentev, Ivan A., Kane, Stephen R., Hill, Michelle L., Rabus, Markus, Esquerdo, Gilbert A., Berlind, Perry, Collins, Karen A., Murawski, Gabriel, Sallam, Nezar Hazam, Aitken, Michael M., Massey, Bob, Ricker, George R., Vanderspek, Roland, Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Barclay, Thomas, Caldwell, Douglas A., Dragomir, Diana, Doty, John P., Glidden, Ana, Tenenbaum, Peter, Torres, Guillermo, Twicken, Joseph D., Villanueva Jr, Steven
Exoplanets can evolve significantly between birth and maturity, as their atmospheres, orbits, and structures are shaped by their environment. Young planets ($<$1 Gyr) offer an opportunity to probe the critical early stages of this evolution, where pl
Externí odkaz:
http://arxiv.org/abs/2005.00047
We review efforts to describe the approach to chiral symmetry restoration in neutron matter from the low-energy realization of QCD, chiral effective field theory.
Comment: Contribution to the Gerry Brown 90th birthday memorial book published by
Comment: Contribution to the Gerry Brown 90th birthday memorial book published by
Externí odkaz:
http://arxiv.org/abs/1609.07109
Autor:
Rockcliffe, Keighley, Newton, Elisabeth, Youngblood, Allison, Gao, Peter, Plavchan, Peter, Lopez, Eric
AU Mic is an M1Ve star in the \(\beta\) Pic moving group with a characterized age of 23 \(\pm\) 3 Myr. At 9.79 \(\pm\) 0.04 pc, it is one of the closest pre-main sequence stars to Earth. TESS has led to the discovery of two exoplanets transiting AU M
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7c6d6cd9f67ff6b033c6e622c193db87
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