Arid
DOI10.3847/1538-3881/aba530
HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert*
Jordan, A.; Bakos, G. A.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Espinoza, N.; Hartman, J. D.; Henning, Th; Mancini, L.; Penev, K.; Rabus, M.; Sarkis, P.; Suc, V; de Val-Borro, M.; Zhou, G.; Butler, R. P.; Teske, J.; Crane, J.; Shectman, S.; Tan, T. G.; Thompson, I; Wallace, J. J.; Lazar, J.; Papp, I; Sari, P.
通讯作者Jordan, A
来源期刊ASTRONOMICAL JOURNAL
ISSN0004-6256
EISSN1538-3881
出版年2020
卷号160期号:5
英文摘要We report the discovery of two transiting Neptunes by the HATSouth survey. The planet HATS-37Ab has a mass of 0.099 +/- 0.042 MJ (31.5.+/-.13.4M(circle dot)) and a radius of 0.606 +/- 0.016 R-J, and is on a P = 4.3315 day orbit around a V = 12.266 +/- 0.030 mag, 0.843(-0.012)(+0.017)M(circle dot) star with a radius of 0.877(-0.012)(+0.019) R-circle dot We also present evidence that the star HATS-37A has an unresolved stellar companion HATS-37B, with a photometrically estimated mass of 0.654 +/- 0.033.M-circle dot The planet HATS-38b has a mass of 0.074. 0.011MJ (23.5 +/- 3.5M(circle dot)) and a radius of 0.614 +/- 0.017 R-J, and is on a P = 4.3750 day orbit around a V = 12.411 +/- 0.030 mag, 0.890(-0.012)(+0.016) M-circle dot star with a radius of 1.105 +/- 0.016.R-circle dot Both systems appear to be old, with isochrone-based ages of 11.46(-1.45)(+0.79) Gyr, and 11.89 +/- 0.60 Gyr, respectively. Both HATS-37Ab and HATS-38b lie in the Neptune desert and are thus examples of a population with a low occurrence rate. They are also among the lowest-mass planets found from ground-based wide-field surveys to date.
英文关键词Exoplanets Hot Neptunes
类型Article
语种英语
开放获取类型Bronze, Green Submitted
收录类别SCI-E
WOS记录号WOS:000584931800001
WOS关键词SPECTROGRAPH ; ALGORITHM
WOS类目Astronomy & Astrophysics
WOS研究方向Astronomy & Astrophysics
资源类型期刊论文
条目标识符http://119.78.100.177/qdio/handle/2XILL650/327259
作者单位[Jordan, A.; Brahm, R.; Suc, V] Univ Adolfo Ibanez, Fac Ingn & Ciencias, Av Diagonal Tones 2640, Santiago, Chile; [Jordan, A.; Brahm, R.] Millenium Inst Astrophys, Santiago, Chile; [Bakos, G. A.; Bhatti, W.; Csubry, Z.; Hartman, J. D.; Wallace, J. J.] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA; [Bakos, G. A.] Konkoly Observ Budapest, Budapest, Hungary; [Bayliss, D.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England; [Bento, J.] Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia; [Espinoza, N.] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA; [Henning, Th; Mancini, L.; Sarkis, P.] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany; [Mancini, L.] Univ Roma Tor Vergata, Dept Phys, Via Ric Sci 1, I-00133 Rome, Italy; [Mancini, L.] INAF Astrophys Observ Turin, Via Osservatorio 20, I-10025 Pino Torinese, Italy; [Penev, K.] Univ Texas Dallas, Dept Phys, Richardson, TX 75080 USA; [Rabus, M.] Las Cumbres Observ Global ...
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Jordan, A.,Bakos, G. A.,Bayliss, D.,et al. HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert*[J],2020,160(5).
APA Jordan, A..,Bakos, G. A..,Bayliss, D..,Bento, J..,Bhatti, W..,...&Sari, P..(2020).HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert*.ASTRONOMICAL JOURNAL,160(5).
MLA Jordan, A.,et al."HATS-37Ab and HATS-38b: Two Transiting Hot Neptunes in the Desert*".ASTRONOMICAL JOURNAL 160.5(2020).
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