TOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite

Vista sencilla de ítem
dc.contributor.authorBrahm, Rafael
dc.contributor.authorNielsen, Louise D.
dc.contributor.authorWittenmyer, Robert A.
dc.contributor.authorWang, Songhu
dc.contributor.authorRodriguez, Joseph E.
dc.contributor.authorEspinoza, Néstor
dc.contributor.authorJones, Matías I.
dc.contributor.authorJordán, Andrés
dc.contributor.authorHenning, Thomas
dc.contributor.authorHobson, Melissa
dc.contributor.authorKossakowski, Diana
dc.contributor.authorRojas, Felipe
dc.contributor.authorSarkis, Paula
dc.contributor.authorSchlecker, Martin
dc.contributor.authorTrifonov, Trifon
dc.contributor.authorShahaf, Sahar
dc.contributor.authorRicker, George
dc.contributor.authorVanderspek, Roland
dc.contributor.authorLatham, David W.
dc.contributor.authorSeager, Sara
dc.contributor.authorWinn, Joshua N.
dc.contributor.authorJenkins, Jon M.
dc.contributor.authorAddison, Brett C.
dc.contributor.authorBakos, Gáspár Á.
dc.contributor.authorBhatti, Waqas
dc.contributor.authorBayliss, Daniel
dc.contributor.authorBerlind, Perry
dc.contributor.authorBieryla, Allyson
dc.contributor.authorBouchy, Francois
dc.contributor.authorBowler, Brendan P.
dc.contributor.authorBriceño, César
dc.contributor.authorBrown, Timothy M.
dc.contributor.authorBryant, Edward M.
dc.contributor.authorCaldwell, Douglas A.
dc.contributor.authorCharbonneau, David
dc.contributor.authorCollins, Karen A.
dc.contributor.authorDavis, Allen B.
dc.contributor.authorEsquerdo, Gilbert A.
dc.contributor.authorFulton, Benjamin J.
dc.contributor.authorGuerrero, Natalia M.
dc.contributor.authorHenze, Christopher E.
dc.contributor.authorHogan, Aleisha
dc.contributor.authorHorner, Jonathan
dc.contributor.authorHuang, Chelsea X.
dc.contributor.authorIrwin, Jonathan
dc.contributor.authorKane, Stephen R.
dc.contributor.authorKielkopf, John
dc.contributor.authorMann. Andrew W.
dc.contributor.authorMazeh, Tsevi
dc.contributor.authorMccormac, James
dc.contributor.authorMccully, Curtis
dc.contributor.authorMengel, Matthew W.
dc.contributor.authorMireles, Ismael
dc.contributor.authorOkumura, Jack
dc.contributor.authorPlavchan, Peter
dc.contributor.authorQuinn, Samuel N.
dc.contributor.authorRabus, Markus
dc.contributor.authorSaesen, Sophie
dc.contributor.authorSchlieder, Joshua E.
dc.contributor.authorSegransan, Damien
dc.contributor.authorShiao, Bernie
dc.contributor.authorShporer, Avi
dc.contributor.authorSiverd, Robert J.
dc.contributor.authorStassun, Keivan G.
dc.contributor.authorSuc, Vincent
dc.contributor.authorTan, Thiam-Guan
dc.contributor.authorTorres, Pascal
dc.contributor.authorTinney, Chris G.
dc.contributor.authorUdry, Stephane
dc.contributor.authorVanzi, Leonardo
dc.contributor.authorVezie, Michael
dc.contributor.authorVines, Jose I.
dc.contributor.authorVuckovic, Maja
dc.contributor.authorWright, Duncan J.
dc.contributor.authorYahalomi, Daniel A.
dc.contributor.authorZapata, Abner
dc.contributor.authorZhang, Hui
dc.contributor.authorZiegler, Carl
dc.date.accessioned2022-11-30T02:46:12Z
dc.date.available2022-11-30T02:46:12Z
dc.date.issued2020
dc.description.abstractWe present the discovery of two new 10 day period giant planets from the Transiting Exoplanet Survey Satellite mission, whose masses were precisely determined using a wide diversity of ground-based facilities. TOI-481 b and TOI-892 b have similar radii (0.99 ± 0.01 ${R}_{{\rm{J}}}$ and 1.07 ± 0.02 ${R}_{{\rm{J}}}$, respectively), and orbital periods (10.3311 days and 10.6266 days, respectively), but significantly different masses (1.53 ± 0.03 ${M}_{{\rm{J}}}$ versus 0.95 ± 0.07 ${M}_{{\rm{J}}}$, respectively). Both planets orbit metal-rich stars ($[\mathrm{Fe}/{\rm{H}}]$ = $+0.26\pm 0.05$ dex and $[\mathrm{Fe}/{\rm{H}}]$ = $+0.24\pm 0.05$ for TOI-481 and TOI-892, respectively) but at different evolutionary stages. TOI-481 is a ${M}_{\star }$ = 1.14 ± 0.02 ${M}_{\odot }$, ${R}_{\star }$ = 1.66 ± 0.02 ${R}_{\odot }$ G-type star (${T}_{\mathrm{eff}}$ = $5735\pm 72$ K), that with an age of 6.7 Gyr, is in the turn-off point of the main sequence. TOI-892 on the other hand, is a F-type dwarf star (${T}_{\mathrm{eff}}$ = $6261\pm 80$ K), which has a mass of ${M}_{\star }$ = 1.28 ± 0.03 ${M}_{\odot }$ and a radius of ${R}_{\star }$ = 1.39 ± 0.02 ${R}_{\odot }$. TOI-481 b and TOI-892 b join the scarcely populated region of transiting gas giants with orbital periods longer than 10 days, which is important to constrain theories of the formation and structure of hot Jupiters.en_ES
dc.facultadFacultad de Cienciasen_ES
dc.file.nameBrahm_Toi2020.pdf
dc.identifier.citationRafael Brahm et al 2020 AJ 160 235en_ES
dc.identifier.doihttps://doi.org/10.3847/1538-3881/abba3b
dc.identifier.urihttp://repositoriobibliotecas.uv.cl/handle/uvscl/7250
dc.languageen
dc.publisherAmerican Astronomical Society (Aas)
dc.rights© 2021. The American Astronomical Society. All rights reserved.
dc.sourceThe Astronomical Journal
dc.subjectEXOPLANET DETECTION METHODSen_ES
dc.subjectTRANSIT PHOTOMETRYen_ES
dc.subjectRADIAL VELOCITYen_ES
dc.subjectEXOPLANET ASTRONOMYen_ES
dc.titleTOI-481 b and TOI-892 b: Two Long-period Hot Jupiters from the Transiting Exoplanet Survey Satellite
dc.typeArticulo
uv.departamentoInstituto de Fisica y Astronomia

Archivos

Bloque original
Mostrando 1 - 1 de 1
Miniatura
Nombre:
Brahm_Toi2020.pdf
Tamaño:
6.19 MB
Formato:
Adobe Portable Document Format
Descargar

Colecciones

Artículos investigadores UV