SWEET-Cat: A view on the planetary mass-radius relation

被引：0

作者：

Sousa, S.G. ^{[1
]}

Adibekyan, V. ^{[1
]}

Delgado-Mena, E. ^{[1
]}

Santos, N.C. ^{[1
,2
]}

Rojas-Ayala, B. ^{[3
]}

Barros, S.C.C. ^{[1
]}

Demangeon, O.D.S. ^{[1
,2
]}

Hoyer, S. ^{[4
]}

Israelian, G. ^{[5
]}

Mortier, A. ^{[6
]}

Soares, B.M.T.B. ^{[1
,2
]}

Tsantaki, M. ^{[7
]}

机构：

[1] Instituto de Astrofísica e Ciências Do Espaço, Universidade Do Porto, CAUP, Rua das Estrelas, Porto,4150-762, Portugal

[2] Departamento de Física e Astronomia, Faculdade de Ciências, Universidade Do Porto, Rua do Campo Alegre, Porto,4169-007, Portugal

[3] Instituto de Alta Investigación, Universidad de Tarapacá, Casilla 7D, Arica, Chile

[4] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

[5] Instituto de Astrofísica de Canarias, Tenerife, La Laguna,38200, Spain

[6] School of Physics & Astronomy, University of Birmingham, Birmingham, Edgbaston,B15 2TT, United Kingdom

[7] INAF - Osservatorio Astrofisico di Arcetri, Largo Enrico Fermi 5, Firenze,50125, Italy

来源：

Astronomy and Astrophysics | 1600年 / 691卷

关键词：

Aims. SWEET-Cat (Stars With ExoplanETs Catalog) was originally introduced in 2013; and since then; the number of confirmed exoplanets has increased significantly. A crucial step for a comprehensive understanding of these new worlds is the precise and homogeneous characterization of their host stars. Methods. We used a large number of high-resolution spectra to continue the addition of new stellar parameters for planet-hosting stars in SWEET-Cat following the new detection of exoplanets listed both in the Extrasolar Planets Encyclopedia and in the NASA exoplanet archive. We obtained high-resolution spectra for a significant number of these planet-hosting stars; either observed by our team or collected through public archives. For FGK stars; the spectroscopic stellar parameters were derived for the spectra following the same homogeneous process using ARES+MOOG as for the previous SWEET-Cat releases. The stellar properties were combined with the planet properties to study possible correlations that could shed more light on the star-planet connection studies. Results. We have increased the number of stars with homogeneous parameters by 232 (∼25% - from 959 to 1191). We focus on the exoplanets that have had both mass and radius determined to review the mass-radius relation; and we find results consistent with the ones previously reported in the literature. For the massive planets; we also revisit the radius anomaly; confirming a metallicity correlation for the radius anomaly already hinted at in previous results. © The Authors 2024;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

Journal article (JA)

引用

共 50 条

[31] ON THE MASS-RADIUS RELATION OF LATE M-DWARFS
CAILLAULT, JP
PATTERSON, J
ASTRONOMICAL JOURNAL, 1990, 100 (03): : 825 - 829
[32] Mass-radius relation for fractal aggregates of polydisperse particles
Gmachowski, L
COLLOIDS AND SURFACES A-PHYSICOCHEMICAL AND ENGINEERING ASPECTS, 2003, 224 (1-3) : 45 - 52
[33] Mass-Radius Relation of Strongly Magnetized White Dwarfs
Bera, Prasanta
Bhattacharya, Dipankar
20TH EUROPEAN WHITE DWARF WORKSHOP, 2017, 509 : 395 - 400
[34] UNDERSTANDING THE MASS-RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION
Lopez, Eric D.
Fortney, Jonathan J.
ASTROPHYSICAL JOURNAL, 2014, 792 (01):
[35] Mass-Radius relation of love-mass stars revisited with the VLTI
Demory, B. -O.
Segransan, D.
Forveille, T.
Queloz, D.
Delfosse, X.
Perrier, C.
COOL STARS, STELLAR SYSTEMS AND THE SUN, 2009, 1094 : 792 - +
[36] Effective interactions of hyperons and mass-radius relation of neutron stars
Lim, Yeunhwan
Lee, Chang-Hwan
Oh, Yongseok
PHYSICAL REVIEW D, 2018, 97 (02)
[37] Mass-radius relation for strongly magnetized white dwarfs with anisotropy
Moussa, Mohamed
ANNALS OF PHYSICS, 2017, 385 : 347 - 357
[38] The white dwarf mass-radius relation with Gaia, Hubble and FUSE
Joyce, Simon R. G.
Barstow, Martin A.
Casewell, Sarah L.
Holberg, Jay B.
Bond, Howard E.
ASTROMETRY AND ASTROPHYSICS IN THE GAIA SKY, 2018, 12 (S330): : 301 - 304
[39] Mass-radius relation for magnetized white dwarfs from SDSS
Karinkuzhi, Drisya
Mukhopadhyay, Banibrata
Wickramasinghe, Dayal
Tout, Christopher A.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2024, 529 (04) : 4577 - 4584
[40] The Planetary Mass-Radius Relation and Its Dependence on Orbital Period as Measured by Transit Timing Variations and Radial Velocities
Mills, Sean M.
Mazeh, Tsevi
ASTROPHYSICAL JOURNAL LETTERS, 2017, 839 (01)

← 1 2 3 4 5 →