Search Results - "Konings, Thomas"

Can we predict a delirium after cardiac surgery? A validation study of a delirium risk checklist by ten Broeke, Miarca, Koster, Sandra, Konings, Thomas, Hensens, Ab G, van der Palen, Job

“…Background: Delirium is a common temporary mental disorder that often occurs in patients who undergo cardiac surgery. It is important to prevent the negative…”
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Grid of pseudo-2D chemistry models for tidally locked exoplanets – II. The role of photochemistry by Baeyens, Robin, Konings, Thomas, Venot, Olivia, Carone, Ludmila, Decin, Leen

“…ABSTRACT Photochemistry is expected to change the chemical composition of the upper atmospheres of irradiated exoplanets through the dissociation of species,…”
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SO2, silicate clouds, but no CH4 detected in a warm Neptune by Dyrek, Achrène, Min, Michiel, Decin, Leen, Bouwman, Jeroen, Crouzet, Nicolas, Mollière, Paul, Lagage, Pierre-Olivier, Konings, Thomas, Tremblin, Pascal, Güdel, Manuel, Pye, John, Waters, Rens, Henning, Thomas, Vandenbussche, Bart, Ardevol Martinez, Francisco, Argyriou, Ioannis, Ducrot, Elsa, Heinke, Linus, van Looveren, Gwenael, Absil, Olivier, Barrado, David, Baudoz, Pierre, Boccaletti, Anthony, Cossou, Christophe, Coulais, Alain, Edwards, Billy, Gastaud, René, Glasse, Alistair, Glauser, Adrian, Greene, Thomas P., Kendrew, Sarah, Krause, Oliver, Lahuis, Fred, Mueller, Michael, Olofsson, Goran, Patapis, Polychronis, Rouan, Daniel, Royer, Pierre, Scheithauer, Silvia, Waldmann, Ingo, Whiteford, Niall, Colina, Luis, van Dishoeck, Ewine F., Östlin, Göran, Ray, Tom P., Wright, Gillian

“…WASP-107b is a warm (approximately 740 K) transiting planet with a Neptune-like mass of roughly 30.5  M ⊕ and Jupiter-like radius of about 0.94  R J (refs.  1…”
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SO 2 , silicate clouds, but no CH 4 detected in a warm Neptune by Dyrek, Achrène, Min, Michiel, Decin, Leen, Bouwman, Jeroen, Crouzet, Nicolas, Mollière, Paul, Lagage, Pierre-Olivier, Konings, Thomas, Tremblin, Pascal, Güdel, Manuel, Pye, John, Waters, Rens, Henning, Thomas, Vandenbussche, Bart, Ardevol Martinez, Francisco, Argyriou, Ioannis, Ducrot, Elsa, Heinke, Linus, van Looveren, Gwenael, Absil, Olivier, Barrado, David, Baudoz, Pierre, Boccaletti, Anthony, Cossou, Christophe, Coulais, Alain, Edwards, Billy, Gastaud, René, Glasse, Alistair, Glauser, Adrian, Greene, Thomas P, Kendrew, Sarah, Krause, Oliver, Lahuis, Fred, Mueller, Michael, Olofsson, Goran, Patapis, Polychronis, Rouan, Daniel, Royer, Pierre, Scheithauer, Silvia, Waldmann, Ingo, Whiteford, Niall, Colina, Luis, van Dishoeck, Ewine F, Östlin, Göran, Ray, Tom P, Wright, Gillian

“…WASP-107b is a warm (approximately 740 K) transiting planet with a Neptune-like mass of roughly 30.5 M and Jupiter-like radius of about 0.94 R (refs.  ), whose…”
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Impact of stellar flares on the chemical composition and transmission spectra of gaseous exoplanets orbiting M dwarfs by Konings, Thomas, Baeyens, Robin, Decin, Leen

“…A&A 667, A15 (2022) Stellar flares of active M dwarfs can affect the atmospheric composition of close-orbiting gas giants, and can result in time-dependent…”
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A new pathway to SO$_2$: Revealing the NUV driven sulfur chemistry in hot gas giants by de Gruijter, Wiebe, Tsai, Shang-Min, Min, Michiel, Waters, Rens, Konings, Thomas, Decin, Leen

“…Context. Photochemistry is a key process driving planetary atmospheres away from local thermodynamic equilibrium. Recent observations of the H$_2$ dominated…”
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Grid of pseudo-2D chemistry models for tidally locked exoplanets -- II. The role of photochemistry by Baeyens, Robin, Konings, Thomas, Venot, Olivia, Carone, Ludmila, Decin, Leen

“…Photochemistry is expected to change the chemical composition of the upper atmospheres of irradiated exoplanets through the dissociation of species, such as…”
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3D simulations of AGB stellar winds -- II. Ray-tracer implementation and impact of radiation on the outflow morphology by Esseldeurs, Mats, Siess, Lionel, De Ceuster, Frederik, Homan, Ward, Malfait, Jolien, Maes, Silke, Konings, Thomas, Ceulemans, Thomas, Decin, Leen

“…A&A 674, A122 (2023) Stars with an initial mass below ~ 8 Msun evolve through the asymptotic giant branch (AGB) phase, during which they develop strong stellar…”
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SO$_2$, silicate clouds, but no CH$_4$ detected in a warm Neptune by Dyrek, Achrène, Min, Michiel, Decin, Leen, Bouwman, Jeroen, Crouzet, Nicolas, Mollière, Paul, Lagage, Pierre-Olivier, Konings, Thomas, Tremblin, Pascal, Güdel, Manuel, Pye, John, Waters, Rens, Henning, Thomas, Vandenbussche, Bart, Martinez, Francisco Ardevol, Argyriou, Ioannis, Ducrot, Elsa, Heinke, Linus, Van Looveren, Gwenael, Absil, Olivier, Barrado, David, Baudoz, Pierre, Boccaletti, Anthony, Cossou, Christophe, Coulais, Alain, Edwards, Billy, Gastaud, René, Glasse, Alistair, Glauser, Adrian, Greene, Thomas P, Kendrew, Sarah, Krause, Oliver, Lahuis, Fred, Mueller, Michael, Olofsson, Goran, Patapis, Polychronis, Rouan, Daniel, Royer, Pierre, Scheithauer, Silvia, Waldmann, Ingo, Whiteford, Niall, Colina, Luis, van Dishoeck, Ewine F, Greve, Thomas, Ostlin, Göran, Ray, Tom P, Wright, Gillian

“…WASP-107b is a warm ($\sim$740 K) transiting planet with a Neptune-like mass of $\sim$30.5 $M_{\oplus}$ and Jupiter-like radius of $\sim$0.94 $R_{\rm J}$,…”
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