NOWAK, Grzegorz, Enric PALLE, Davide GANDOLFI, Hans J. DEEG, Teruyuki HIRANO, Oscar BARRAGAN, Masayuki KUZUHARA, Fei DAI, Rafael LUQUE, Carina M. PERSSON, Malcolm FRIDLUND, Marshall C. JOHNSON, Judith KORTH, John H. LIVINGSTON, Sascha GRZIWA, Savita MATHUR, Artie P. HATZES, Jorge PRIETO-ARRANZ, David NESPRAL, Diego HIDALGO, Maria HJORTH, Simon ALBRECHT, Vincent VAN EYLEN, Kristine W. F. LAM, William D. COCHRAN, Massimiliano ESPOSITO, Szilard CSIZMADIA, Eike W. GUENTHER, Petr KABATH, Pere BLAY, Rafael BRAHM, Andres JORDAN, Nestor ESPINOZA, Felipe ROJAS, Nuria CASASAYAS BARRIS, Florian RODLER, Roi ALONSO SOBRINO, Juan CABRERA, Ilaria CARLEO, Alexander CHAUSHEV, Jerome DE LEON, Philipp EIGMULLER, Michael ENDL, Anders ERIKSON, Akihiko FUKUI, Iskra GEORGIEVA, Lucia GONZALEZ-CUESTA, Emil KNUDSTRUP, Mikkel N. LUND, Pilar Montanes RODRIGUEZ, Felipe MURGAS, Norio NARITA, Prajwal NIRAULA, Martin PATZOLD, Heike RAUER, Seth REDFIELD, Ignasi RIBAS, Marek SKARKA, Alexis M. S. SMITH a Jano SUBJAK. K2-280 b - a low density warm sub-Saturn around a mildly evolved star. Monthly Notices of the Royal Astronomical Society. Oxford: Oxford University Press, 2020, roč. 497, č. 4, s. 4423-4435. ISSN 0035-8711. Dostupné z: https://dx.doi.org/10.1093/mnras/staa2077.
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Základní údaje
Originální název K2-280 b - a low density warm sub-Saturn around a mildly evolved star
Autoři NOWAK, Grzegorz, Enric PALLE, Davide GANDOLFI, Hans J. DEEG, Teruyuki HIRANO, Oscar BARRAGAN, Masayuki KUZUHARA, Fei DAI, Rafael LUQUE, Carina M. PERSSON, Malcolm FRIDLUND, Marshall C. JOHNSON, Judith KORTH, John H. LIVINGSTON, Sascha GRZIWA, Savita MATHUR, Artie P. HATZES, Jorge PRIETO-ARRANZ, David NESPRAL, Diego HIDALGO, Maria HJORTH, Simon ALBRECHT, Vincent VAN EYLEN, Kristine W. F. LAM, William D. COCHRAN, Massimiliano ESPOSITO, Szilard CSIZMADIA, Eike W. GUENTHER, Petr KABATH, Pere BLAY, Rafael BRAHM, Andres JORDAN, Nestor ESPINOZA, Felipe ROJAS, Nuria CASASAYAS BARRIS, Florian RODLER, Roi ALONSO SOBRINO, Juan CABRERA, Ilaria CARLEO, Alexander CHAUSHEV, Jerome DE LEON, Philipp EIGMULLER, Michael ENDL, Anders ERIKSON, Akihiko FUKUI, Iskra GEORGIEVA, Lucia GONZALEZ-CUESTA, Emil KNUDSTRUP, Mikkel N. LUND, Pilar Montanes RODRIGUEZ, Felipe MURGAS, Norio NARITA, Prajwal NIRAULA, Martin PATZOLD, Heike RAUER, Seth REDFIELD, Ignasi RIBAS, Marek SKARKA (203 Česká republika, domácí), Alexis M. S. SMITH a Jano SUBJAK.
Vydání Monthly Notices of the Royal Astronomical Society, Oxford, Oxford University Press, 2020, 0035-8711.
Další údaje
Originální jazyk angličtina
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Stát vydavatele Velká Británie a Severní Irsko
Utajení není předmětem státního či obchodního tajemství
WWW URL
Impakt faktor Impact factor: 5.287
Kód RIV RIV/00216224:14310/20:00117711
Organizační jednotka Přírodovědecká fakulta
Doi http://dx.doi.org/10.1093/mnras/staa2077
UT WoS 000587739300034
Klíčová slova anglicky techniques: photometric; techniques: radial velocities; techniques: spectroscopic; planets and satellites: detection; stars: individual: (EPIC 216494238; K2-280)
Štítky rivok
Příznaky Mezinárodní význam, Recenzováno
Změnil Změnila: Mgr. Marie Šípková, DiS., učo 437722. Změněno: 12. 1. 2021 15:31.
Anotace
We present an independent discovery and detailed characterization of K2-280 b, a transiting low density warm sub-Saturn in a 19.9-d moderately eccentric orbit (e = 0.35(-0.04)(+0.05)) from K2 campaign 7. A joint analysis of high precision HARPS, HARPS-N, and FIES radial velocity measurements and K2 photometric data indicates that K2-280 b has a radius of R-b = 7.50 +/- 0.44 R-circle plus and a mass of M-b = 37.1 +/- 5.6 M-circle plus, yielding a mean density of rho(b) = 0.48(-0.10)(+0.13) g cm(-3). The host star is a mildly evolved G7 star with an effective temperature of T-eff = 5500 +/- 100 K, a surface gravity of log g(star) = 4.21 +/- 0.05 (cgs), and an iron abundance of [Fe/H] = 0.33 +/- 0.08 dex, and with an inferred mass of M-star = 1.03 +/- 0.03 M-circle dot and a radius of R-star = 1.28 +/- 0.07 R-circle dot. We discuss the importance of K2-280 b for testing formation scenarios of sub-Saturn planets and the current sample of this intriguing group of planets that are absent in the Solar system.
VytisknoutZobrazeno: 25. 4. 2024 19:42