Zobrazeno 1 - 10
of 135
pro vyhledávání: '"Rizzuto, Aaron"'
Autor:
Thao, Pa Chia, Mann, Andrew W., Feinstein, Adina D., Gao, Peter, Thorngren, Daniel, Rotman, Yoav, Welbanks, Luis, Brown, Alexander, Duvvuri, Girish M., France, Kevin, Longo, Isabella, Sandoval, Angeli, Schneider, P. Christian, Wilson, David J., Youngblood, Allison, Vanderburg, Andrew, Barber, Madyson G., Wood, Mackenna L., Batalha, Natasha E., Kraus, Adam L., Murray, Catriona Anne, Newton, Elisabeth R., Rizzuto, Aaron, Tofflemire, Benjamin M., Tsai, Shang-Min, Bean, Jacob L., Berta-Thompson, Zachory K., Evans-Soma, Thomas M., Froning, Cynthia S., Kempton, Eliza M. -R., Miguel, Yamila, Pineda, J. Sebastian
The characterization of young planets (< 300 Myr) is pivotal for understanding planet formation and evolution. We present the 3-5$\mu$m transmission spectrum of the 17 Myr, Jupiter-size ($R$ $\sim$10$R_{\oplus}$) planet, HIP 67522 b, observed with JW
Externí odkaz:
http://arxiv.org/abs/2409.16355
Young stellar populations provide a powerful record that traces millions of years of star formation history in the solar neighborhood. Using a revised form of the SPYGLASS young star identification methodology, we produce an expanded census of nearby
Externí odkaz:
http://arxiv.org/abs/2306.08150
Autor:
Kerr, Ronan, Kraus, Adam L., Murphy, Simon J., Krolikowski, Daniel M., Bedding, Timothy R., Rizzuto, Aaron C.
The study of young associations is essential for building a complete record of local star formation processes. The Fornax-Horologium association (FH), including the $\chi^1$ Fornacis cluster, represents one of the nearest young stellar populations to
Externí odkaz:
http://arxiv.org/abs/2211.00123
Autor:
Kerr, Ronan, Kraus, Adam L., Murphy, Simon J., Krolikowski, Daniel M., Offner, Stella S. R., Tofflemire, Benjamin M., Rizzuto, Aaron C.
Young stellar populations provide a record of past star formation, and by establishing their members' dynamics and ages, it is possible to reconstruct the full history of star formation events. Gaia has greatly expanded the number of accessible stell
Externí odkaz:
http://arxiv.org/abs/2209.12959
Autor:
Dupuy, Trent J., Kraus, Adam L., Kratter, Kaitlin M., Rizzuto, Aaron C., Mann, Andrew W., Huber, Daniel, Ireland, Michael J.
Planet formation is often considered in the context of one circumstellar disk around one star. Yet stellar binary systems are ubiquitous, and thus a substantial fraction of all potential planets must form and evolve in more complex, dynamical environ
Externí odkaz:
http://arxiv.org/abs/2202.00013
Autor:
Mann, Andrew W., Wood, Mackenna L., Schmidt, Stephen P., Barber, Madyson G., Owen, James E., Tofflemire, Benjamin M., Newton, Elisabeth R., Mamajek, Eric E., Bush, Jonathan L., Mace, Gregory N., Kraus, Adam L., Thao, Pa Chia, Vanderburg, Andrew, Llama, Joe, Johns-Krull, Christopher M., Prato, L., Stahl, Asa G., Tang, Shih-Yun, Fields, Matthew J., Collins, Karen A., Collins, Kevin I., Gan, Tianjun, Jensen, Eric L. N., Kamler, Jacob, Schwarz, Richard P., Furlan, Elise, Gnilka, Crystal L., Howell, Steve B., Lester, Kathryn V., Owens, Dylan A., Suarez, Olga, Mekarnia, Djamel, Guillot, Tristan, Abe, Lyu, Triaud, Amaury H. M. J., Johnson, Marshall C., Milburn, Reilly P., Rizzuto, Aaron C., Quinn, Samuel N., Kerr, Ronan, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, Sara, Winn, Joshua N., Jenkins, Jon M., Guerrero, Natalia M., Shporer, Avi, Schlieder, Joshua E., McLean, Brian, Wohler, Bill
Publikováno v:
AJ 163 156 (2022)
Mature super-Earths and sub-Neptunes are predicted to be $\simeq$Jovian radius when younger than 10 Myr. Thus, we expect to find 5-15$R_\oplus$ planets around young stars even if their older counterparts harbor none. We report the discovery and valid
Externí odkaz:
http://arxiv.org/abs/2110.09531
Autor:
Heitzmann, Alexis, Zhou, George, Quinn, Samuel N., Marsden, Stephen C., Wright, Duncan, Petit, Pascal, Vanderburg, Andrew M., Bouma, Luke G., Mann, Andrew W., Rizzuto, Aaron C.
HIP 67522 b is a 17 Myr old, close-in ($P_{orb} = 6.96$ d), Jupiter-sized ($R = 10\,R_{\oplus}$) transiting planet orbiting a Sun like star in the Sco-Cen OB association. We present our measurement of the system's projected orbital obliquity via two
Externí odkaz:
http://arxiv.org/abs/2109.04174
The Taurus-Auriga complex is the prototypical low-mass star forming region, and provides a unique testbed of the star formation process, which left observable imprints on the spatial, kinematic, and temporal structure of its stellar population. Tauru
Externí odkaz:
http://arxiv.org/abs/2105.13370
Young stellar associations hold a star formation record that can persist for millions of years, revealing the progression of star formation long after the dispersal of the natal cloud. To identify nearby young stellar populations that trace this prog
Externí odkaz:
http://arxiv.org/abs/2105.09338
Autor:
Tofflemire, Benjamin M., Rizzuto, Aaron C., Newton, Elisabeth R., Kraus, Adam L., Mann, Andrew W., Vanderburg, Andrew, Nelson, Tyler, Hawkins, Keith, Wood, Mackenna L., Zhou, George, Quinn, Samuel N., Howell, Steve B., Collins, Karen A., Schwarz, Richard P., Stassun, Keivan G., Bouma, Luke G., Essack, Zahra, Osborn, Hugh, Boyd, Patricia T., Furesz, Gabor, Glidden, Ana, Twicken, Joseph D., Wohler, Bill, McLean, Brian, Ricker, George R., Vanderspek, Roland, Latham, David W., Seager, S., Winn, Joshua N., Jenkins, Jon M.
The detection and characterization of young planetary systems offers a direct path to study the processes that shape planet evolution. We report on the discovery of a sub-Neptune-size planet orbiting the young star HD 110082 (TOI-1098). Transit event
Externí odkaz:
http://arxiv.org/abs/2102.06066