Zobrazeno 1 - 10
of 214
pro vyhledávání: '"Ray, Tom"'
Autor:
Schwarz, Kamber R., Samland, Matthias, Olofsson, Göran, Henning, Thomas, Sellek, Andrew, Güdel, Manuel, Tabone, Benoît, Kamp, Inga, Lagage, Pierre-Olivier, van Dishoeck, Ewine F., Garatti, Alessio Caratti o, Glauser, Adrian M., Ray, Tom P., Arabhavi, Aditya M., Christiaens, Valentin, Franceschi, Riccardo, Gasman, Danny, Grant, Sierra L., Kanwar, Jayatee, Kaeufer, Till, Kurtovic, Nicolas T., Perotti, Giulia, Temmink, Milou, Vlasblom, Marissa
The removal of angular momentum from protostellar systems drives accretion onto the central star and may drive the dispersal of the protoplanetary disk. Winds and jets can contribute to removing angular momentum from the disk, though the dominant pro
Externí odkaz:
http://arxiv.org/abs/2409.11176
Autor:
Mâlin, Mathilde, Boccaletti, Anthony, Perrot, Clément, Baudoz, Pierre, Rouan, Daniel, Lagage, Pierre-Olivier, Waters, Rens, Güdel, Manuel, Henning, Thomas, Vandenbussche, Bart, Absil, Olivier, Barrado, David, Bouwman, Jeroen, Cossou, Christophe, Decin, Leen, Glauser, Adrian M., Pye, John, Olofsson, Goran, Glasse, Alistair, Lahuis, Fred, Patapis, Polychronis, Royer, Pierre, Scheithauer, Silvia, Whiteford, Niall, Serabyn, Eugene, Choquet, Elodie, Colina, Luis, Ostlin, Göran, van Dishoeck, Ewine F., Ray, Tom P., Wright, Gillian
Mid-infrared imaging of exoplanets and disks is now possible with the coronagraphs of the MIRI on the JWST. This wavelength range unveils new features of young directly imaged systems and allows us to obtain new constraints for characterizing the atm
Externí odkaz:
http://arxiv.org/abs/2408.16843
Autor:
Franceschi, Riccardo, Henning, Thomas, Tabone, Benoît, Perotti, Giulia, Garatti, Alessio Caratti o, Bettoni, Giulio, van Dishoeck, Ewine F., Kamp, Inga, Absil, Olivier, Güdel, Manuel, Olofsson, Göran, Waters, L. B. F. M., Arabhavi, Aditya M., Christiaens, Valentin, Gasman, Danny, Grant, Sierra L., Jang, Hyerin, Rodgers-Lee, Donna, Samland, Matthias, Schwarz, Kamber, Temmink, Milou, Barrado, David, Boccaletti, Anthony, Geers, Vincent, Lagage, Pierre-Olivier, Pantin, Eric, Ray, Tom P., Scheithauer, Silvia, Vandenbussche, Bart, Wright, Gillian
This work aims to measure the mass accretion rate, the accretion luminosity, and more generally the physical conditions of the warm emitting gas in the inner disk of the very low-mass star 2MASS-J16053215-1933159. We investigate the source mid-infrar
Externí odkaz:
http://arxiv.org/abs/2404.11942
Autor:
Delabrosse, Valentin, Dougados, Catherine, Cabrit, Sylvie, Tabone, Benoit, Tychoniec, Lukasz, Ray, Tom, Podio, Linda, McClure, Melissa
Publikováno v:
A&A 688, A173 (2024)
The origin and impact of outflows on proto-planetary disks and planet formation are key open questions. DG Tau B, a Class I protostar with a structured disk and a striking rotating conical CO outflow, recently identified with ALMA as one of the best
Externí odkaz:
http://arxiv.org/abs/2403.19400
Autor:
Temmink, Milou, van Dishoeck, Ewine F., Grant, Sierra L., Tabone, Benoit, Gasman, Danny, Christiaens, Valentin, Samland, Matthias, Argyriou, Ioannis, Perotti, Giulia, Guedel, Manuel, Henning, Thomas, Lagage, Pierre-Oliver, Abergel, Alian, Absil, Olivier, Barrado, David, Garatti, Alessio Caratti o, Glauser, Adrian M., Kamp, Inga, Lahuis, Fred, Olofsson, Goeran, Ray, Tom P., Scheithauer, Silvia, Vandenbussche, Bart, Waters, Rens L. B. F. M., Arabhavi, Aditya M., Jang, Hyerin, Kanwar, Jayatee, Morales-Calderon, Maria, Rodgers-Lee, Donna, Schreiber, Juergen, Schwarz, Kamber, Colina, Luis
The MRS mode of the JWST-MIRI instrument has been shown to be a powerful tool to characterise the molecular gas emission of the inner region of planet-forming disks. Here, we analyse the spectrum of the compact T-Tauri disk DR Tau, which is complemen
Externí odkaz:
http://arxiv.org/abs/2403.13591
Autor:
Henning, Thomas, Kamp, Inga, Samland, Matthias, Arabhavi, Aditya M., Kanwar, Jayatee, van Dishoeck, Ewine F., Guedel, Manuel, Lagage, Pierre-Olivier, Waelkens, Christoffel, Abergel, Alain, Absil, Olivier, Barrado, David, Boccaletti, Anthony, Bouwman, Jeroen, Garatti, Alessio Caratti o, Geers, Vincent, Glauser, Adrian M., Lahuis, Fred, Nehme, Cyrine, Olofsson, Goeran, Pantin, Eric, Ray, Tom P., Vandenbussche, Bart, Waters, L. B. F. M., Wright, Gillian, Christiaens, Valentin, Franceschi, Riccardo, Gasman, Danny, Guadarrama, Rodrigo, Jang, Hyerin, Morales-Calderon, Maria, Pawellek, Nicole, Perotti, Giulia, Rodgers-Lee, Donna, Schreiber, Juergen, Schwarz, Kamber, Tabone, Benoit, Temmink, Milou, Vlasblom, Marissa, Colina, Luis, Greve, Thomas R., Oestlin, Goeran
The study of protoplanetary disks has become increasingly important with the Kepler satellite finding that exoplanets are ubiquitous around stars in our galaxy and the discovery of enormous diversity in planetary system architectures and planet prope
Externí odkaz:
http://arxiv.org/abs/2403.09210
Autor:
De Lucia, Mario, Ulbricht, Gerhard, Baldwin, Eoin, Piercy, Jack, Bracken, Colm, Creaner, Oisin, Ray, Tom
Publikováno v:
AIP Advances 13, 125026 (2023)
This paper describes the energy resolution of Microwave Kinetic Inductance Detectors (MKIDs), and models some limiting factors to it. Energy resolution is a measure of the smallest possible difference in energy of the impinging photons, Delta E, that
Externí odkaz:
http://arxiv.org/abs/2402.10108
Autor:
Schwarz, Kamber R., Henning, Thomas, Christiaens, Valentin, Gasman, Danny, Samland, Matthias, Perotti, Giulia, Jang, Hyerin, Grant, Sierra L., Tabone, Benoit, Morales-Calderon, Maria, Kamp, Inga, van Dishoeck, Ewine F., Gudel, Manuel, Lagage, Pierre-Olivier, Argyriou, Ioannis, Barrado, David, Garatti, Alessio Caratti o, Glauser, Adrian M., Ray, Tom P., Vandenbussche, Bart, Waters, L. B. F. M., Arabhavi, Aditya M., Kanwar, Jayatee, Olofsson, Goran, Rodgers-Lee, Donna, Schreiber, Jurgen, Temmink, Milou
SY Cha is a T Tauri star surrounded by a protoplanetary disk with a large cavity seen in the millimeter continuum but has the spectral energy distribution (SED) of a full disk. Here we report the first results from JWST-MIRI Medium Resolution Spectro
Externí odkaz:
http://arxiv.org/abs/2312.07135
Autor:
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 $R_{\rm J}$, whose extended atmosphere is eroding. Previous observations showed evidence for water vapour an
Externí odkaz:
http://arxiv.org/abs/2311.12515
Autor:
Barrado, David, Mollière, Paul, Patapis, Polychronis, Min, Michiel, Tremblin, Pascal, Martinez, Francisco Ardevol, Whiteford, Niall, Vasist, Malavika, Argyriou, Ioannis, Samland, Matthias, Lagage, Pierre-Olivier, Decin, Leen, Waters, Rens, Henning, Thomas, Morales-Calderón, María, Guedel, Manuel, Vandenbussche, Bart, Absil, Olivier, Baudoz, Pierre, Boccaletti, Anthony, Bouwman, Jeroen, Cossou, Christophe, Coulais, Alain, Crouzet, Nicolas, Gastaud, René, Glasse, Alistair, Glauser, Adrian M., Kamp, Inga, Kendrew, Sarah, Krause, Oliver, Lahuis, Fred, Mueller, Michael, Olofsson, Göran, Pye, John, Rouan, Daniel, Royer, Pierre, Scheithauer, Silvia, Waldmann, Ingo, Colina, Luis, van Dishoeck, Ewine F., Ray, Tom, Östlin, Göran, Wright, Gillian
Brown dwarfs serve as ideal laboratories for studying the atmospheres of giant exoplanets on wide orbits as the governing physical and chemical processes in them are nearly identical. Understanding the formation of gas giant planets is challenging, o
Externí odkaz:
http://arxiv.org/abs/2311.08054