Results 51 to 60 of about 10,029 (146)
An Ultra-Short Period Super-Earth and Sub-Neptune Spanning the Radius Valley Orbiting the Kinematic Thick Disk Star TOI-2345
A crucial chemical link between stars and their orbiting exoplanets is thought to exist. If universal, this connection could affect the formation and evolution of all planets.Smith, Alexis M S, Buder, Maximilian, Rauer, Heike, Scandariato, Gaetano, Venturini, Julia, Rando, Nicola, Brandeker, Alexis, Fortier, Andrea, Cubillos, Patricio E, Ziegler, Carl, Baumjohann, Wolfgang, Heitzmann, Alexis, Szabó, Gyula M, Deleuil, Magali, Wilson, Thomas G, Fridlund, Malcolm, Queloz, Didier, Ratti, Francesco, Hasiba, Johann, Derekas, Aliz, Piotto, Giampaolo, Isaak, Kate G, Barrado, David, Borsato, Luca, Santos, Nuno C, Magrin, Demetrio, Ségransan, Damien, Benz, Willy, Lam, Kristine W F, Vivien, Hugo G, Kiss, Laszlo L, Eschen, Yoshi Nike Emilia, Barros, Susana C C, Bárczy, Tamas, Bonfanti, Andrea, Egger, Jo Ann, Demangeon, Olivier D S, Deline, Adrien, Gandolfi, Davide, Keller, Tatiana, Stalport, Manu, Demory, Brice-Olivier, Cameron, Andrew Collier, Ehrenreich, David, Goeke, Robert, Peter, Gisbert, Csizmadia, Szilard, Correia, Alexandre C M, Pollacco, Don, Ulmer-Moll, Soléne, Olofsson, Göran, Davies, Melvyn B, Ribas, Ignasi, Piazza, Daniele, Caldwell, Douglas A, Mordasini, Christoph, Jenkins, Jon M, Günther, Maximilian N, Fossati, Luca, Broeg, Christopher, Wolf, Sebastian, Laskar, Jacques, Sulis, Sophia, Merín, Bruno, Van Grootel, Valérie, Maxted, Pierre F L, Gillon, Michaël, Osborn, Hugh P, Watanabe, David, Ottensamer, Roland, Erikson, Anders, Lendl, Monika, Ragazzoni, Roberto, Farinato, Jacopo, Korth, Judith, Villaver, Eva, Pallé, Enric, Helling, Ch, Etangs, Alain Lecavelier des, Nascimbeni, Valerio, Shporer, Avi, Castro-González, Amadeo, Mustill, Alexander James, Walton, Nicholas A, Billot, Nicolas, Güdel, Manuel, Alibert, Yann, Pagano, Isabella, Simon, Attila E, Leleu, Adrien, Edwards, Billy, Kitzmann, Daniel, Sousa, Sérgio G, Persson, Carina M, Gazeas, Kosmas, Alonso, Roi, Udry, Stéphane +96 morecore +1 more sourceThree hot Jupiters transiting K-dwarfs with significant heavy element masses
Context. Despite predictions from planetary population synthesis models indicating that such systems should be exceedingly rare, short-period gas giants do exist around low-mass stars (Teff < 4965 K), albeit at lower frequency than around hotter stars ...M. Battley, Relles, H. M., Y. G. C. Frensch, Timmermans, M., B. Tofflemire, Stassun, K. G., Radford, D. J., B. Lavie, Jenkins, J. M., Pepe, F., A. Revol, C. N. Watkins, M. Gillon, E. Jehin, Law, N., M. Steiner, F. Pepe, Battley, M., Udry, S., Pozuelos, F. J., C. Farret Jentink, S. G. Sousa, F. J. Pozuelos, Collins, K. A., Tan, T.-G., Watkins, C. N., H. Chakraborty, J. P. Faria, N. C. Santos, Jehin, E., D. W. Latham, Daylan, T., K. G. Stassun, Sousa, S. G., G. Lo Curto, E. Fontanet, Fontanet, E., Strakhov, I. A., D. J. Radford, T.-G. Tan, Frensch, Y. G. C., Ulmer-Moll, S., Mann, A. W., F. Bouchy, J. M. Jenkins, Chakraborty, H., T. Daylan, C. Hellier, Revol, A., N. Grieves, Parc, L., M. Timmermans, Popowicz, A., Vanderspek, R., H. M. Relles, Fridén, E., G. Ricker, K. A. Collins, S. Tavella, Seager, S., Furesz, G., S. Seager, Santos, N. C., Lo Curto, G., Vaulato, V., S. Ulmer-Moll, J. N. Winn, Tavella, S., A. W. Mann, G. Furesz, F. Murgas, Grieves, N., Faria, J. P., Latham, D. W., V. Vaulato, A. Popowicz, Tofflemire, B., N. Law, I. A. Strakhov, Barkaoui, K., M. Shinde, Ricker, G., Murgas, F., L. Parc, Gillon, M., Evans, P., Ceva, W., L. K. W. Kwok, Hellier, C., Winn, J. N., Steiner, M., E. Palle, Kwok, L. K. W., P. Evans, W. Ceva, Bouchy, F., Farret Jentink, C., Lavie, B., R. Vanderspek, Ziegler, C., K. Barkaoui, S. Udry, C. Ziegler, Palle, E., E. Fridén, Shinde, M. +105 morecore +1 more sourceA possible misaligned orbit for the young planet AU Mic c
The AU Microscopii planetary system is only 24 Myr old, and its geometry may provide clues about the early dynamical history of planetary systems. Here, we present the first measurement of the Rossiter-McLaughlin effect for the warm sub-Neptune AU Mic c, Ulmer, B, Steinberger, M, Lam, K W F, Demory, B.-O, Southworth, R, Wilson, T G, Lafarga, M, Peter, G, Kriskovics, L, Aigrain, S, Ottensamer, R, Barrado, D, Mordasini, C, Csizmadia, Sz, Egger, J A, Günther, M N, Demangeon, O D S, Fossati, L, Baumjohann, W, Fortier, A, Maxted, P F L, Walton, N A, Billot, N, Pagano, I, Szabó, Gy M, Davies, M B, Gill, S, Alonso, R, Güdel, M, Garai, Z, Owen, J E, Borsato, L, Merín, B, Barros, S C C, Gillon, M, Gandolfi, D, Olofsson, G, Etangs, A Lecavelier des, Sousa, S G, Ehrenreich, D, McCormac, J, Villaver, E, Korth, J, Brandeker, A, Derekas, A, Fridlund, M, Cretignier, M, Kiss, L L, Benz, W, Bryant, E M, Broeg, C, Barragán, O, Bergomi, M, Bayliss, D, Queloz, D, Bárczy, T, Yu, H, Rauer, H, Sulis, S, Gazeas, K, Erikson, A, Ribas, I, Nielsen, L D, Cegla, H M, Santos, N C, Alibert, Y, Deline, A, Rando, N, Edwards, B, Van Grootel, V, O’Brien, S M, Scandariato, G, Wheatley, P J, Boldog, A, Winn, J N, Deleuil, M, Correia, A C M, Stalport, M, Heitzmann, A, Meech, A, Nascimbeni, V, Pollacco, D, Magrin, D, Laskar, J, Smith, A M S, Isaak, K G, Helling, Ch, Simon, A E, Pallé, E, Piotto, G, Ragazzoni, R, Klein, B, Lendl, M, Cameron, A Collier, Doyle, L, Venturini, J, Cubillos, P E, Ségransan, D, Piazza, D, Ulmer-Moll, S, Udry, S +100 morecore +1 more sourceArchitecture of TOI-561 planetary system
We present new observations from CHEOPS (CHaracterising ExOPlanet Satellite) and TESS (Transiting Exoplanet Survey Satellite) to clarify the architecture of the planetary system hosted by the old Galactic thick disc star TOI-561.Bárczy, T, Mantovan, G, Lam, K W F, Rauer, H, Sulis, S, Gazeas, K, Sicilia, D, Zingales, T, Florén, H -G, Wilson, T G, Erikson, A, Ribas, I, Peter, G, Santos, N C, Alibert, Y, Deline, A, Rando, N, Hooton, M J, Edwards, B, Ottensamer, R, Scandariato, G, Mordasini, C, Egger, J A, Csizmadia, Sz, Günther, M N, Adibekyan, V, Fossati, L, Demangeon, O D S, Baumjohann, W, Fortier, A, Winn, J N, Beck, T, Leonardi, P, Deleuil, M, Correia, A C M, Maxted, P F L, Walton, N A, Billot, N, Demory, B -O, Pagano, I, Davies, M B, Stalport, M, Szabó, Gy M, Alonso, R, Heitzmann, A, Nascimbeni, V, Güdel, M, Ratti, F, Nardiello, D, Lacedelli, G, Borsato, L, Pollacco, D, Barros, S C C, Magrin, D, Gillon, M, Laskar, J, Gandolfi, D, Olofsson, G, Sousa, S G, Ehrenreich, D, Smith, A M S, Villaver, E, Isaak, K G, Korth, J, Helling, Ch, Bonfanti, A, Brandeker, A, Lecavelier des Etangs, A, Simon, A E, Derekas, A, Fridlund, M, Pallé, E, Van Grootel, V, Piotto, G, Luque, R, Salmon, S, Ragazzoni, R, Wolf, S, Lendl, M, Kiss, L L, Benz, W, Cameron, A Collier, Venturini, J, Broeg, C, Buder, M, Cubillos, P E, Ségransan, D, Barrado Navascues, D, Malavolta, L, Ulmer-Moll, S, Udry, S, Queloz, D +91 morecore +1 more sourceSimultaneous Measurement of Local Pulse Wave Velocities in Radial Arteries Using a Soft Sensor Based on the Fiber Bragg Grating Technique
MicromachinesArterial stiffness has been proved to be an important parameter in the evaluation of cardiovascular diseases, and Pulse Wave Velocity (PWV) is a strong indicator of arterial stiffness. Compared to regional PWV (PWV among different arteries), local PWV (PWV within a single artery) outstands in providing higher precision in indicating arterial properties,Jing Wang, Zhukun Wang, Zijun Zhang, Peiyun Li, Han Pan, Yong Ren, Tuo Hou, Chengbo Wang, Chiew-Foong Kwong, Bei Zhang, Sen Yang, Jing Bie +11 moreopenaire +3 more sources
