TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm
Jupiter Unlikely to Have Originated from High-eccentricity
Migration

J 2022

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration

TRAN, Quang H.; Brendan P. BOWLER; Michael ENDL; William D. COCHRAN; Phillip J. MACQUEEN et. al.

Základní údaje

Originální název

TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration

Autoři

TRAN, Quang H.; Brendan P. BOWLER; Michael ENDL; William D. COCHRAN; Phillip J. MACQUEEN; Davide GANDOLFI; Carina M. PERSSON; Malcolm FRIDLUND; Enric PALLE; Grzegorz NOWAK; Hans J. DEEG; Rafael LUQUE; John H. LIVINGSTON; Petr KABATH; Marek SKARKA (203 Česká republika, domácí); Jan SUBJAK; Steve B. HOWELL; Simon H. ALBRECHT; Karen A. COLLINS; Massimiliano ESPOSITO; Van Eylen VINCENT; Sascha GRZIWA; Elisa GOFFO; Chelsea X. HUANG; Jon M. JENKINS; Marie KARJALAINEN; Raine KARJALAINEN; Emil KNUDSTRUP; Judith KORTH; Kristine W. F. LAM; David W. LATHAM; Alan M. LEVINE; H. L. M. OSBORNE; Samuel N. QUINN; Seth REDFIELD; George R. RICKER; S. SEAGER; Luisa Maria SERRANO; Alexis M. S. SMITH; Joseph D. TWICKEN a Joshua N. WINN

Vydání

Astronomical Journal, IOP Publishing Ltd, 2022, 0004-6256

Další údaje

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

Odkazy

URL URL

Impakt faktor

Impact factor: 5.300

Kód RIV

RIV/00216224:14310/22:00127833

Organizační jednotka

Přírodovědecká fakulta

DOI

http://dx.doi.org/10.3847/1538-3881/ac5c4f

UT WoS

000785598300001

EID Scopus

2-s2.0-85129611035

Klíčová slova anglicky

planetary systems; planets and satellites: detection; stars: individual (TOI-1670)

Štítky

rivok

Příznaky

Mezinárodní význam, Recenzováno

Změněno: 10. 1. 2023 09:47, Mgr. Marie Novosadová Šípková, DiS.

Anotace

V originále

We report the discovery of two transiting planets around the bright (V = 9.9 mag) main-sequence F7 star TOI-1670 by the Transiting Exoplanet Survey Satellite. TOI-1670 b is a sub-Neptune (R-b = 2.06(-0.15)(+0.19) R-circle plus) on a 10.9 day orbit, and TOI-1670 c is a warm Jupiter (R-c= 0.987(-0.025)(+0.025) R-Jup) on a 40.7 day orbit. Using radial velocity observations gathered with the Tull Coude Spectrograph on the Harlan J. Smith telescope and HARPS-N on the Telescopio Nazionale Galileo, we find a planet mass of M-c = 0.63(-0.08)(+0.09) M(Jup )for the outer warm Jupiter, implying a mean density of rho(c) = 0.81(-0.11)(+0.13) g cm(-3). The inner sub-Neptune is undetected in our radial velocity data (M-b < 0.13 M-Jup at the 99% confidence level). Multiplanet systems like TOI-1670 hosting an outer warm Jupiter on a nearly circular orbit (l(e) = 0.09(-0.04)(+0.05)) and one or more inner coplanar planets are more consistent with "gentle" formation mechanisms such as disk migration or in situ formation rather than high-eccentricity migration. Of the 11 known systems with a warm Jupiter and a smaller inner companion, eight (73%) are near a low-order mean-motion resonance, which can be a signature of migration. TOI-1670 joins two other systems (27% of this subsample) with period commensurabilities greater than 3, a common feature of in situ formation or halted inward migration. TOI-1670 and the handful of similar systems support a diversity of formation pathways for warm Jupiters.

Citovat

TRAN, Quang H.; Brendan P. BOWLER; Michael ENDL; William D. COCHRAN; Phillip J. MACQUEEN; Davide GANDOLFI; Carina M. PERSSON; Malcolm FRIDLUND; Enric PALLE; Grzegorz NOWAK; Hans J. DEEG; Rafael LUQUE; John H. LIVINGSTON; Petr KABATH; Marek SKARKA; Jan SUBJAK; Steve B. HOWELL; Simon H. ALBRECHT; Karen A. COLLINS; Massimiliano ESPOSITO; Van Eylen VINCENT; Sascha GRZIWA; Elisa GOFFO; Chelsea X. HUANG; Jon M. JENKINS; Marie KARJALAINEN; Raine KARJALAINEN; Emil KNUDSTRUP; Judith KORTH; Kristine W. F. LAM; David W. LATHAM; Alan M. LEVINE; H. L. M. OSBORNE; Samuel N. QUINN; Seth REDFIELD; George R. RICKER; S. SEAGER; Luisa Maria SERRANO; Alexis M. S. SMITH; Joseph D. TWICKEN a Joshua N. WINN. TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration. Astronomical Journal. IOP Publishing Ltd, 2022, roč. 163, č. 5, s. 1-16. ISSN 0004-6256. Dostupné z: https://dx.doi.org/10.3847/1538-3881/ac5c4f.

@article{2245093,
   author = {Tran, Quang H. and Bowler, Brendan P. and Endl, Michael and Cochran, William D. and MacQueen, Phillip J. and Gandolfi, Davide and Persson, Carina M. and Fridlund, Malcolm and Palle, Enric and Nowak, Grzegorz and Deeg, Hans J. and Luque, Rafael and Livingston, John H. and Kabath, Petr and Skarka, Marek and Subjak, Jan and Howell, Steve B. and Albrecht, Simon H. and Collins, Karen A. and Esposito, Massimiliano and Vincent, Van Eylen and Grziwa, Sascha and Goffo, Elisa and Huang, Chelsea X. and Jenkins, Jon M. and Karjalainen, Marie and Karjalainen, Raine and Knudstrup, Emil and Korth, Judith and Lam, Kristine W. F. and Latham, David W. and Levine, Alan M. and Osborne, H. L. M. and Quinn, Samuel N. and Redfield, Seth and Ricker, George R. and Seager, S. and Serrano, Luisa Maria and Smith, Alexis M. S. and Twicken, Joseph D. and Winn, Joshua N.},
   article_number = {5},
   doi = {http://dx.doi.org/10.3847/1538-3881/ac5c4f},
   keywords = {planetary systems; planets and satellites: detection; stars: individual (TOI-1670)},
   language = {eng},
   issn = {0004-6256},
   journal = {Astronomical Journal},
   title = {TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration},
   url = {https://iopscience.iop.org/article/10.3847/1538-3881/ac5c4f},
   volume = {163},
   year = {2022}
}

TY  - JOUR
ID  - 2245093
AU  - Tran, Quang H. - Bowler, Brendan P. - Endl, Michael - Cochran, William D. - MacQueen, Phillip J. - Gandolfi, Davide - Persson, Carina M. - Fridlund, Malcolm - Palle, Enric - Nowak, Grzegorz - Deeg, Hans J. - Luque, Rafael - Livingston, John H. - Kabath, Petr - Skarka, Marek - Subjak, Jan - Howell, Steve B. - Albrecht, Simon H. - Collins, Karen A. - Esposito, Massimiliano - Vincent, Van Eylen - Grziwa, Sascha - Goffo, Elisa - Huang, Chelsea X. - Jenkins, Jon M. - Karjalainen, Marie - Karjalainen, Raine - Knudstrup, Emil - Korth, Judith - Lam, Kristine W. F. - Latham, David W. - Levine, Alan M. - Osborne, H. L. M. - Quinn, Samuel N. - Redfield, Seth - Ricker, George R. - Seager, S. - Serrano, Luisa Maria - Smith, Alexis M. S. - Twicken, Joseph D. - Winn, Joshua N.
PY  - 2022
TI  - TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration
JF  - Astronomical Journal
VL  - 163
IS  - 5
SP  - 1-16
EP  - 1-16
PB  - IOP Publishing Ltd
SN  - 00046256
KW  - planetary systems
KW  - planets and satellites: detection
KW  - stars: individual (TOI-1670)
UR  - https://iopscience.iop.org/article/10.3847/1538-3881/ac5c4f
N2  - We report the discovery of two transiting planets around the bright (V = 9.9 mag) main-sequence F7 star TOI-1670 by the Transiting Exoplanet Survey Satellite. TOI-1670 b is a sub-Neptune (R-b = 2.06(-0.15)(+0.19) R-circle plus) on a 10.9 day orbit, and TOI-1670 c is a warm Jupiter (R-c= 0.987(-0.025)(+0.025) R-Jup) on a 40.7 day orbit. Using radial velocity observations gathered with the Tull Coude Spectrograph on the Harlan J. Smith telescope and HARPS-N on the Telescopio Nazionale Galileo, we find a planet mass of M-c = 0.63(-0.08)(+0.09) M(Jup )for the outer warm Jupiter, implying a mean density of rho(c) = 0.81(-0.11)(+0.13) g cm(-3). The inner sub-Neptune is undetected in our radial velocity data (M-b < 0.13 M-Jup at the 99% confidence level). Multiplanet systems like TOI-1670 hosting an outer warm Jupiter on a nearly circular orbit (l(e) = 0.09(-0.04)(+0.05)) and one or more inner coplanar planets are more consistent with "gentle" formation mechanisms such as disk migration or in situ formation rather than high-eccentricity migration. Of the 11 known systems with a warm Jupiter and a smaller inner companion, eight (73%) are near a low-order mean-motion resonance, which can be a signature of migration. TOI-1670 joins two other systems (27% of this subsample) with period commensurabilities greater than 3, a common feature of in situ formation or halted inward migration. TOI-1670 and the handful of similar systems support a diversity of formation pathways for warm Jupiters.
ER  -

TRAN, Quang H.; Brendan P. BOWLER; Michael ENDL; William D. COCHRAN; Phillip J. MACQUEEN; Davide GANDOLFI; Carina M. PERSSON; Malcolm FRIDLUND; Enric PALLE; Grzegorz NOWAK; Hans J. DEEG; Rafael LUQUE; John H. LIVINGSTON; Petr KABATH; Marek SKARKA; Jan SUBJAK; Steve B. HOWELL; Simon H. ALBRECHT; Karen A. COLLINS; Massimiliano ESPOSITO; Van Eylen VINCENT; Sascha GRZIWA; Elisa GOFFO; Chelsea X. HUANG; Jon M. JENKINS; Marie KARJALAINEN; Raine KARJALAINEN; Emil KNUDSTRUP; Judith KORTH; Kristine W. F. LAM; David W. LATHAM; Alan M. LEVINE; H. L. M. OSBORNE; Samuel N. QUINN; Seth REDFIELD; George R. RICKER; S. SEAGER; Luisa Maria SERRANO; Alexis M. S. SMITH; Joseph D. TWICKEN a Joshua N. WINN. TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration. \textit{Astronomical Journal}. IOP Publishing Ltd, 2022, roč.~163, č.~5, s.~1-16. ISSN~0004-6256. Dostupné z: https://dx.doi.org/10.3847/1538-3881/ac5c4f.

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