PERSSON, Carina M., Szilard CSIZMADIA, Alexander J. MUSTILL, Malcolm FRIDLUND, Artie P. HATZES, Grzegorz NOWAK, Iskra GEORGIEVA, Davide GANDOLFI, Melvyn B. DAVIES, John H. LIVINGSTON, Enric PALLE, Pilar RODRIGUEZ, Michael ENDL, Teruyuki HIRANO, Jorge PRIETO-ARRANZ, Judith KORTH, Sascha GRZIWA, Massimiliano ESPOSITO, Simon ALBRECHT, Marshall C. JOHNSON, Oscar BARRAGAN, Hannu PARVIAINEN, Eylen Vincent VAN, Roi SOBRINO, Paul G. BECK, Juan CABRERA, Ilaria CARLEO, William D. COCHRAN, Fei DAI, Hans J. DEEG, Jerome P. DE LEON, Philipp EIGMULLER, Anders ERIKSON, Akai FUKUI, Lucia GONZALEZ-CUESTA, Eike W. GUENTHER, Diego HIDALGO, Maria HJORTH, Petr KABÁTH, Emil KNUDSTRUP, Nobuhiko KUSAKABE, Kristine W. F. LAM, Mikkel N. LUND, Rafael LUQUE, Savita MATHUR, Felipe MURGAS, Norio NARITA, David NESPRAL, Prajwal NIRAULA, A. O. Henrik OLOFSSON, Martin PATZOLD, Heike RAUER, Seth REDFIELD, Ignasi RIBAS, Marek SKARKA, Alexis M. S. SMITH, Jan SUBJAK a Motohide TAMURA. Greening of the brown-dwarf desert EPIC 212036875b: a 51 M-J object in a 5-day orbit around an F7V star. ASTRONOMY & ASTROPHYSICS. Les Ulis: EDP SCIENCES S A, 2019, roč. 628, AUG, s. 1-14. ISSN 1432-0746. Dostupné z: https://dx.doi.org/10.1051/0004-6361/201935505.
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Základní údaje
Originální název Greening of the brown-dwarf desert EPIC 212036875b: a 51 M-J object in a 5-day orbit around an F7V star
Autoři PERSSON, Carina M. (garant), Szilard CSIZMADIA, Alexander J. MUSTILL, Malcolm FRIDLUND, Artie P. HATZES, Grzegorz NOWAK, Iskra GEORGIEVA, Davide GANDOLFI, Melvyn B. DAVIES, John H. LIVINGSTON, Enric PALLE, Pilar RODRIGUEZ, Michael ENDL, Teruyuki HIRANO, Jorge PRIETO-ARRANZ, Judith KORTH, Sascha GRZIWA, Massimiliano ESPOSITO, Simon ALBRECHT, Marshall C. JOHNSON, Oscar BARRAGAN, Hannu PARVIAINEN, Eylen Vincent VAN, Roi SOBRINO, Paul G. BECK, Juan CABRERA, Ilaria CARLEO, William D. COCHRAN, Fei DAI, Hans J. DEEG, Jerome P. DE LEON, Philipp EIGMULLER, Anders ERIKSON, Akai FUKUI, Lucia GONZALEZ-CUESTA, Eike W. GUENTHER, Diego HIDALGO, Maria HJORTH, Petr KABÁTH (203 Česká republika), Emil KNUDSTRUP, Nobuhiko KUSAKABE, Kristine W. F. LAM, Mikkel N. LUND, Rafael LUQUE, Savita MATHUR, Felipe MURGAS, Norio NARITA, David NESPRAL, Prajwal NIRAULA, A. O. Henrik OLOFSSON, Martin PATZOLD, Heike RAUER, Seth REDFIELD, Ignasi RIBAS, Marek SKARKA (203 Česká republika, domácí), Alexis M. S. SMITH, Jan SUBJAK a Motohide TAMURA.
Vydání ASTRONOMY & ASTROPHYSICS, Les Ulis, EDP SCIENCES S A, 2019, 1432-0746.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Francie
Utajení není předmětem státního či obchodního tajemství
WWW Full Text
Impakt faktor Impact factor: 5.636
Kód RIV RIV/00216224:14310/19:00111909
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.1051/0004-6361/201935505
UT WoS 000480314000002
Klíčová slova anglicky planetary systems; stars: fundamental parameters; stars: individual: EPIC 212036875; techniques: photometric; techniques: radial velocities
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 11. 5. 2020 10:29.
Anotace
Context. Although more than 2000 brown dwarfs have been detected to date, mainly from direct imaging, their characterisation is difficult due to their faintness and model-dependent results. In the case of transiting brown dwarfs, however, it is possible to make direct high-precision observations. Aims. Our aim is to investigate the nature and formation of brown dwarfs by adding a new well-characterised object, in terms of its mass, radius and bulk density, to the currently small sample of less than 20 transiting brown dwarfs. Methods. One brown dwarf candidate was found by the KESPRINT consortium when searching for exoplanets in the K2 space mission Campaign 16 field. We combined the K2 photometric data with a series of multicolour photometric observations, imaging, and radial velocity measurements to rule out false positive scenarios and to determine the fundamental properties of the system. Results. We report the discovery and characterisation of a transiting brown dwarf in a 5.17-day eccentric orbit around the slightly evolved F7V star EPIC 212036875. We find a stellar mass of 1.15 +/- 0.08 M-circle dot, a stellar radius of 1.41 +/- 0.05 R-circle dot, and an age of 5.1 +/- 0.9 Gyr. The mass and radius of the companion brown dwarf are 51 +/- 2 M-J and 0.83 +/- 0.03 R-J, respectively, corresponding to a mean density of 108(-13)(+15) g cm(-3). Conclusions. EPIC 212036875 b is a rare object that resides in the brown-dwarf desert. In the mass-density diagram for planets, brown dwarfs, and stars, we find that all giant planets and brown dwarfs follow the same trend from similar to 0.3 M-J to the turn-over to hydrogen burning stars at similar to 73 M-J. EPIC 212036875 b falls close to the theoretical model for mature H/He dominated objects in this diagram as determined by interior structure models. We argue that EPIC 212036875 b formed via gravitational disc instabilities in the outer part of the disc, followed by a quick migration. Orbital tidal circularisation may have started early in its history for a brief period when the brown dwarf's radius was larger. The lack of spin-orbit synchronisation points to a weak stellar dissipation parameter (Q(star)' greater than or similar to 10(8)), which implies a circularisation timescale of greater than or similar to 23 Gyr, or suggests an interaction between the magnetic and tidal forces of the star and the brown dwarf.
Návaznosti
EF16_027/0008360, projekt VaVNázev: Postdoc@MUNI
VytisknoutZobrazeno: 19. 9. 2024 11:02