Six transiting planets and a chain of Laplace resonances in TOI-178

Autor: Leleu, A, Alibert, Y, Hara, NC, Hooton, MJ, Wilson, TG, Robutel, P, Delisle, JB, Laskar, J, Hoyer, S, Lovis, C, Bryant, EM, Ducrot, E, Cabrera, J, Delrez, L, Acton, JS, Adibekyan, V, Allart, R, Allende Prieto, C, Alonso, R, Alves, D, Anderson, DR, Angerhausen, D, Anglada Escude´, G, Asquier, J, Barrado, D, Barros, SCC, Baumjohann, W, Bayliss, D, Beck, M, Beck, T, Bekkelien, A, Benz, W, Billot, N, Bonfanti, A, Bonfils, X, Bouchy, F, Bourrier, V, Boueundefined, G, Brandeker, A, Broeg, C, Buder, M, Burdanov, A, Burleigh, MR, Baundefinedrczy, T, Cameron, AC, Chamberlain, S, Charnoz, S, Cooke, BF, Corral Van Damme, C, Correia, ACM, Cristiani, S, Damasso, M, Davies, MB, Deleuil, M, Demangeon, ODS, Demory, BO, Di Marcantonio, P, Di Persio, G, Dumusque, X, Ehrenreich, D, Erikson, A, Figueira, P, Fortier, A, Fossati, L, Fridlund, M, Futyan, D, Gandolfi, D, Garciaundefined Munoundefinedz, A, Garcia, LJ, Gill, S, Gillen, E, Gillon, M, Goad, MR, Gonzaundefinedlez Hernaundefinedndez, JI, Guedel, M, Guundefinednther, MN, Haldemann, J, Henderson, B, Heng, K, Hogan, AE, Isaak, K, Jehin, E, Jenkins, JS, Jordaundefinedn, A, Kiss, L, Kristiansen, MH, Lam, K, Lavie, B, Lecavelier Des Etangs, A, Lendl, M, Lillo-Box, J, Lo Curto, G, Magrin, D, Martins, CJAP, Maxted, PFL, McCormac, J, Mehner, A, Micela, G, Molaro, P, Moyano, M

Determining the architecture of multi-planetary systems is one of the cornerstones of understanding planet formation and evolution. Resonant systems are especially important as the fragility of their orbital configuration ensures that no significant

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bf98d005a8f05ccf9eddc5e364a6a48f

An ultrahot Neptune in the Neptune desert

Autor: Jenkins, JS, Díaz, MR, Kurtovic, NT, Espinoza, N, Vines, JI, Rojas, PAP, Brahm, R, Torres, P, Cortés-Zuleta, P, Soto, MG, Lopez, ED, King, GW, Wheatley, PJ, Winn, JN, Ciardi, DR, Ricker, G, Vanderspek, R, Latham, DW, Seager, S, Jenkins, JM, Beichman, CA, Bieryla, A, Burke, CJ, Christiansen, JL, Henze, CE, Klaus, TC, McCauliff, S, Mori, M, Narita, N, Nishiumi, T, Tamura, M, De Leon, JP, Quinn, SN, Villaseñor, JN, Vezie, M, Lissauer, JJ, Collins, KA, Collins, KI, Isopi, G, Mallia, F, Ercolino, A, Petrovich, C, Jordán, A, Acton, JS, Armstrong, DJ, Bayliss, D, Bouchy, F, Belardi, C, Bryant, EM, Burleigh, MR, Cabrera, J, Casewell, SL, Chaushev, A, Cooke, BF, Eigmüller, P, Erikson, A, Foxell, E, Gänsicke, BT, Gill, S, Gillen, E, Günther, MN, Goad, MR, Hooton, MJ, Jackman, JAG, Louden, T, McCormac, J, Moyano, M, Nielsen, LD, Pollacco, D, Queloz, D, Rauer, H, Raynard, L, Smith, AMS, Tilbrook, RH, Titz-Weider, R, Turner, O, Udry, S, Walker, Watson, CA, West, RG, Palle, E, Ziegler, C, Law, N, Mann, AW

About one out of 200 Sun-like stars has a planet with an orbital period shorter than one day: an ultra-short-period planet (Sanchis-ojeda et al. 2014; Winn et al. 2018). All of the previously known ultra-short-period planets are either hot Jupiters,

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::2d8e03a0751428daa54fe9ab2146ed07

NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey

Autor: Tilbrook, RH, Burleigh, MR, Costes, JC, Gill, S, Nielsen, LD, Vines, JI, Queloz, D, Hodgkin, ST, Worters, HL, Goad, MR, Acton, JS, Henderson, BA, Armstrong, DJ, Anderson, DR, Bayliss, D, Bouchy, F, Briegal, JT, Bryant, EM, Casewell, SL, Chaushev, A, Cooke, BF, Eigmüller, P, Gillen, E, Günther, MN, Hogan, A, Jenkins, JS, Lendl, M, McCormac, J, Moyano, M, Raynard, L, Smith, AMS, Udry, S, Watson, CA, West, RG, Wheatley, PJ, Breytenbach, H, Sefako, RR, Thomas, JK, Alves, DR

We report the discovery of four new hot Jupiters with the Next Generation Transit Survey (NGTS). NGTS-15b, NGTS-16b, NGTS-17b, and NGTS-18b are short-period ($P

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::dfe20c4c57b22ddccae47994ca92c9ad

NGTS-10b: The shortest period hot Jupiter yet discovered

Autor: McCormac, J, Gillen, E, Jackman, JAG, Brown, DJA, Bayliss, D, Wheatley, PJ, Anderson, DR, Armstrong, DJ, Bouchy, F, Briegal, JT, Burleigh, MR, Cabrera, J, Casewell, SL, Chaushev, A, Chazelas, B, Chote, P, Cooke, BF, Costes, JC, Csizmadia, S, Eigmüller, P, Erikson, A, Foxell, E, Gänsicke, BT, Goad, MR, Günther, MN, Hodgkin, ST, Hooton, MJ, Jenkins, JS, Lambert, G, Lendl, M, Longstaff, E, Louden, T, Moyano, M, Nielsen, LD, Pollacco, D, Queloz, D, Rauer, H, Raynard, L, Smith, AMS, Smalley, B, Soto, M, Turner, O, Udry, S, Vines, JI, Walker, Watson, CA, West, RG

We report the discovery of a new ultra-short period transiting hot Jupiter from the Next Generation Transit Survey (NGTS). NGTS-10b has a mass and radius of $2.162\,^{+0.092}_{-0.107}$ M$_{\rm J}$ and $1.205\,^{+0.117}_{-0.083}$ R$_{\rm J}$ and orbit

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::03fef83d72d997c1b944912a3ef8ea27

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