Zobrazeno 1 - 2
of 2
pro vyhledávání: '"Marcelo Aron F. Keniger"'
Autor:
Emma Nabbie, Chelsea X. Huang, Jennifer A. Burt, David J. Armstrong, Eric E. Mamajek, Vardan Adibekyan, Sérgio G. Sousa, Eric D. Lopez, Daniel Thorngren, Jorge Fernández Fernández, Gongjie Li, James S. Jenkins, Jose I. Vines, João Gomes da Silva, Robert A. Wittenmyer, Daniel Bayliss, César Briceño, Karen A. Collins, Xavier Dumusque, Keith Horne, Marcelo Aron F. Keniger, Nicholas Law, Jorge Lillo-Box, Shang-Fei Liu, Andrew W. Mann, Louise D. Nielsen, Ares Osborn, Howard M. Relles, José J. Rodrigues, Juan Serrano Bell, Gregor Srdoc, Chris Stockdale, Paul A. Strøm, Cristilyn N. Watkins, Peter J. Wheatley, Duncan J. Wright, George Zhou, Carl Ziegler, George Ricker, Sara Seager, Roland Vanderspek, Joshua N. Winn, Jon M. Jenkins, Michael Fausnaugh, Michelle Kunimoto, Hugh P. Osborn, Samuel N. Quinn, Bill Wohler
Publikováno v:
The Astronomical Journal, Vol 168, Iss 3, p 132 (2024)
The recent discoveries of Neptune-sized ultra-short-period planets (USPs) challenge existing planet formation theories. It is unclear whether these residents of the Hot Neptune Desert have similar origins to smaller, rocky USPs, or if this discrete p
Externí odkaz:
https://doaj.org/article/a9d48ba70414406eb0f96b9084efcfde
Autor:
Ginger Frame, David J Armstrong, Heather M Cegla, Jorge Fernández Fernández, Ares Osborn, Vardan Adibekyan, Karen A Collins, Elisa Delgado Mena, Steven Giacalone, John F Kielkopf, Nuno C Santos, Sérgio G Sousa, Keivan G Stassun, Carl Ziegler, David R Anderson, Susana C C Barros, Daniel Bayliss, César Briceño, Dennis M. Conti, Courtney D Dressing, Xavier Dumusque, Pedro Figueira, William Fong, Samuel Gill, Faith Hawthorn, Jon M Jenkins, Eric L N Jensen, Marcelo Aron F Keniger, David W Latham, Nicholas Law, Jack J Lissauer, Andrew W Mann, Louise D Nielsen, Hugh Osborn, Martin Paegert, Sara Seager, Richard P Schwarz, Avi Shporer, Gregor Srdoc, Paul A Strøm, Joshua N Winn, Peter J Wheatley
Publikováno v:
Monthly Notices of the Royal Astronomical Society.
We present the discovery and confirmation of a transiting hot, bloated Super-Neptune using photometry from TESS and LCOGT and radial velocity measurements from HARPS. The host star TOI-2498 is a V = 11.2, G-type (T$_{eff}$ = 5905 $\pm$ 12K) solar-lik
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2b04d92af08bee2b9b8b8965491ba336
https://doi.org/10.1093/mnras/stad1452
https://doi.org/10.1093/mnras/stad1452