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

NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star

Autor: Grieves, N, Nielsen, LD, Vines, JI, Bryant, EM, Gill, S, Bouchy, F, Lendl, M, Bayliss, D, Eigmueller, P, Segransan, D, Acton, JS, Anderson, DR, Burleigh, MR, Casewell, SL, Chaushev, A, Cooke, BF, Gillen, E, Goad, MR, Günther, MN, Henderson, BA, Hogan, A, Jenkins, JS, Alves, DR, Jordán, A, McCormac, J, Moyano, M, Queloz, D, Raynard, L, Seidel, JV, Smith, AMS, Tilbrook, RH, Udry, S, West, RG, Wheatley, PJ

We report the discovery of the massive hot Jupiter NGTS-13b by the Next Generation Transit Survey (NGTS). The V = 12.7 host star is likely in the subgiant evolutionary phase with log g$_{*}$ = 4.04 $\pm$ 0.05, T$_{eff}$ = 5819 $\pm$ 73 K, M$_{*}$ = 1

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::1e952bd6ebb0f5185dc953a655449038

NGTS-5b: A highly inflated planet offering insights into the sub-Jovian desert

Autor: Eigmüller, P, Chaushev, A, Gillen, E, Smith, A, Nielsen, LD, Turner, O, Csizmadia, S, Smalley, B, Bayliss, D, Belardi, C, Bouchy, F, Burleigh, MR, Cabrera, J, Casewell, SL, Chazelas, B, Cooke, BF, Erikson, A, Gänsicke, BT, Günther, MN, Goad, MR, Grange, A, Jackman, JAG, Jenkins, JS, McCormac, J, Moyano, M, Pollacco, D, Poppenhaeger, K, Queloz, D, Raynard, L, Rauer, H, Udry, S, Walker, Watson, CA, West, RG, Wheatley, PJ

Context: Planetary population analysis gives us insight into formation and evolution processes. For short-period planets, the subJovian desert has been discussed in recent years with regard to the planet population in the mass/period and radius/perio

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::3f99ced2a93bd597a390d4263d03d9cf

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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