دورية أكاديمية

TOI-257b (HD 19916b): a warm sub-saturn orbiting an evolved F-type star

التفاصيل البيبلوغرافية
العنوان: TOI-257b (HD 19916b): a warm sub-saturn orbiting an evolved F-type star
المؤلفون: Addison, Brett C, Wright, Duncan J, Nicholson, Belinda A, Cale, Bryson, Mocnik, Teo, Huber, Daniel, Plavchan, Peter, Wittenmyer, Robert A, Vanderburg, Andrew, Chaplin, William J, Chontos, Ashley, Clark, Jake T, Eastman, Jason D, Ziegler, Carl, Brahm, Rafael, Carter, Bradley D, Clerte, Mathieu, Espinoza, Néstor, Horner, Jonathan, Bentley, John, Jordán, Andrés, Kane, Stephen R, Kielkopf, John F, Laychock, Emilie, Mengel, Matthew W, Okumura, Jack, Stassun, Keivan G, Bedding, Timothy R, Bowler, Brendan P, Burnelis, Andrius, Blanco-Cuaresma, Sergi, Collins, Michaela, Crossfield, Ian, Davis, Allen B, Evensberget, Dag, Heitzmann, Alexis, Howell, Steve B, Law, Nicholas, Mann, Andrew W, Marsden, Stephen C, Matson, Rachel A, O’Connor, James H, Shporer, Avi, Stevens, Catherine, Tinney, C G, Tylor, Christopher, Wang, Songhu, Zhang, Hui, Henning, Thomas, Kossakowski, Diana, Ricker, George, Sarkis, Paula, Schlecker, Martin, Torres, Pascal, Vanderspek, Roland, Latham, David W, Seager, Sara, Winn, Joshua N, Jenkins, Jon M, Mireles, Ismael, Rowden, Pam, Pepper, Joshua, Daylan, Tansu, Schlieder, Joshua E, Collins, Karen A, Collins, Kevin I, Tan, Thiam-Guan, Ball, Warrick H, Basu, Sarbani, Buzasi, Derek L, Campante, Tiago L, Corsaro, Enrico, González-Cuesta, L, Davies, Guy R, de, Almeida, Leandro, do, Nascimento, Jose-Dias, García, Rafael A, Guo, Zhao, Handberg, Rasmus, Hekker, Saskia, Hey, Daniel R, Kallinger, Thomas, Kawaler, Steven D, Kayhan, Cenk, S., Kuszlewicz, James, Lund, Mikkel N, Lyttle, Alexander, Mathur, Savita, Miglio, Andrea, Mosser, Benoit, Nielsen, Martin B, Serenelli, Aldo M, Aguirre, Victor Silva, Themeßl, Nathalie
المساهمون: Addison, Brett C, Wright, Duncan J, Nicholson, Belinda A, Cale, Bryson, Mocnik, Teo, Huber, Daniel, Plavchan, Peter, Wittenmyer, Robert A, Vanderburg, Andrew, Chaplin, William J, Chontos, Ashley, Clark, Jake T, Eastman, Jason D, Ziegler, Carl, Brahm, Rafael, Carter, Bradley D, Clerte, Mathieu, Espinoza, Néstor, Horner, Jonathan, Bentley, John, Jordán, André, Kane, Stephen R, Kielkopf, John F, Laychock, Emilie, Mengel, Matthew W, Okumura, Jack, Stassun, Keivan G, Bedding, Timothy R, Bowler, Brendan P, Burnelis, Andriu, Blanco-Cuaresma, Sergi, Collins, Michaela, Crossfield, Ian, Davis, Allen B, Evensberget, Dag, Heitzmann, Alexi, Howell, Steve B, Law, Nichola, Mann, Andrew W, Marsden, Stephen C, Matson, Rachel A, O’Connor, James H, Shporer, Avi, Stevens, Catherine, Tinney, C G, Tylor, Christopher, Wang, Songhu, Zhang, Hui, Henning, Thoma, Kossakowski, Diana, Ricker, George, Sarkis, Paula, Schlecker, Martin, Torres, Pascal, Vanderspek, Roland, Latham, David W, Seager, Sara, Winn, Joshua N, Jenkins, Jon M, Mireles, Ismael, Rowden, Pam, Pepper, Joshua, Daylan, Tansu, Schlieder, Joshua E, Collins, Karen A, Collins, Kevin I, Tan, Thiam-Guan, Ball, Warrick H, Basu, Sarbani, Buzasi, Derek L, Campante, Tiago L, Corsaro, Enrico, González-Cuesta, L, Davies, Guy R, de Almeida, Leandro, do Nascimento, Jose-Dia, García, Rafael A, Guo, Zhao, Handberg, Rasmu, Hekker, Saskia, Hey, Daniel R, Kallinger, Thoma, Kawaler, Steven D, Kayhan, Cenk, S. Kuszlewicz, Jame, Lund, Mikkel N, Lyttle, Alexander, Mathur, Savita, Miglio, Andrea, Mosser, Benoit, Nielsen, Martin B, Serenelli, Aldo M, Aguirre, Victor Silva, Themeßl, Nathalie
سنة النشر: 2021
المجموعة: IRIS Università degli Studi di Bologna (CRIS - Current Research Information System)
مصطلحات موضوعية: asteroseismology, techniques: photometric, techniques: radial velocitie, techniques: spectroscopic, planetary system, stars: individual (TIC 200723869/TOI-257)
الوصف: We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS and confirmed to be of planetary origin based on radial velocity observations. An analysis of the TESS photometry, the MINERVA-Australis, FEROS, and HARPS radial velocities, and the asteroseismic data of the stellar oscillations reveals that TOI-257b has a mass of M-P = 0.138 +/- 0.023M(J) (43.9 +/- 7.3 M-circle plus), a radius of R-P = 0.639 +/- 0.013 R-J (7.16 +/- 0.15 R-circle plus), bulk density of 0.65(-0.11)(+0.12) (cgs), and period 18.38818(-0.00084)(+0.00085) days. TOI-257b orbits a bright (V = 7.612 mag) somewhat evolved late F-type star with M-* = 1.390 +/- 0.046(Msun), R-* = 1.888 +/- 0.033 R-sun, T-eff = 6075 +/- 90 K, and vsin i = 11.3 +/- 0.5 kms(-1). Additionally, we find hints for a second non-transiting sub-Saturn mass planet on a similar to 71 day orbit using the radial velocity data. This system joins the ranks of a small number of exoplanet host stars (similar to 100) that have been characterized with asteroseismology. Warm sub-Saturns are rare in the known sample of exoplanets, and thus the discovery of TOI-257b is important in the context of future work studying the formation and migration history of similar planetary systems.
نوع الوثيقة: article in journal/newspaper
وصف الملف: ELETTRONICO
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/wos/WOS:000648998800038; volume:502; issue:3; firstpage:3704; lastpage:3722; numberofpages:19; journal:MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY; info:eu-repo/grantAgreement/EC/H2020/772293; http://hdl.handle.net/11585/831675Test; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85103487448; https://academic.oup.com/mnras/article/502/3/3704/6054535Test
DOI: 10.1093/mnras/staa3960
الإتاحة: https://doi.org/10.1093/mnras/staa3960Test
http://hdl.handle.net/11585/831675Test
https://academic.oup.com/mnras/article/502/3/3704/6054535Test
حقوق: info:eu-repo/semantics/openAccess
رقم الانضمام: edsbas.95EE2D8E
قاعدة البيانات: BASE