Zobrazeno 1 - 10
of 387
pro vyhledávání: '"Wright, Chris P."'
Autor:
Wright, Chris J., Thornton, Joel A., Jaeglé, Lyatt, Cao, Yang, Zhu, Yannian, Liu, Jihu, Jones II, Randall, Holzworth, Robert H, Rosenfeld, Daniel, Wood, Robert, Blossey, Peter, Kim, Daehyun
Aerosol interactions with clouds represent a significant uncertainty in our understanding of the Earth system. Deep convective clouds may respond to aerosol perturbations in several ways that have proven difficult to elucidate with observations. Here
Externí odkaz:
http://arxiv.org/abs/2408.07207
Autor:
Norfolk, Brodie J., Maddison, Sarah T., Pinte, Christophe, van der Marel, Nienke, Booth, Richard A., Francis, Logan, Gonzalez, Jean-François, Ménard, François, Wright, Chris M., van der Plas, Gerrit, Garg, Himanshi
The origin of the inner dust cavities observed in transition discs remains unknown. The segregation of dust and size of the cavity is expected to vary depending on which clearing mechanism dominates grain evolution. We present the results from the Di
Externí odkaz:
http://arxiv.org/abs/2102.02316
Akademický článek
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Akademický článek
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Autor:
Barnes, Peter, Li, Dan, Telesco, Charles, Tanakul, Nahathai, Mariñas, Naibí, Wright, Chris, Packham, Chris, Pantin, Eric, Roche, Patrick, Hough, James
We report new imaging polarimetry observations of the Galactic compact HII region K3-50 using CanariCam at the Gran Telescopio Canarias. We use a standard polarimetric analysis technique, first outlined by Aitken, to decompose the observed polarisati
Externí odkaz:
http://arxiv.org/abs/1506.02173
Autor:
Casassus, Simon, Wright, Chris, Marino, Sebastian, Maddison, Sarah T., Wootten, Al, Roman, Pablo, Perez, Sebastian, Pinilla, Paola, Wyatt, Mark, Moral, Victor, Menard, Francois, Christiaens, Valentin, Cieza, Lucas, van der Plas, Gerrit
Publikováno v:
2015, ApJ, 812, 126
A pathway to the formation of planetesimals, and eventually giant planets, may occur in concentrations of dust grains trapped in pressure maxima. Dramatic crescent-shaped dust concentrations have been seen in recent radio images at sub-mm wavelengths
Externí odkaz:
http://arxiv.org/abs/1505.07743
Akademický článek
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Autor:
Vogt, Steven S., Radovan, Matthew, Kibrick, Robert, Butler, R. Paul, Alcott, Barry, Allen, Steve, Arriagada, Pamela, Bolte, Mike, Burt, Jennifer, Cabak, Jerry, Chloros, Kostas, Cowley, David, Deich, William, Dupraw, Brian, Earthman, Wayne, Epps, Harland, Faber, Sandra, Fischer, Debra, Gates, Elinor, Hilyard, David, Holden, Brad, Johnston, Ken, Keiser, Sandy, Kanto, Dick, Katsuki, Myra, Laiterman, Lee, Lanclos, Kyle, Laughlin, Greg, Lewis, Jeff, Lockwood, Chris, Lynam, Paul, Marcy, Geoffrey, McLean, Maureen, Miller, Joe, Misch, Tony, Peck, Michael, Pfister, Terry, Phillips, Andrew, Rivera, Eugenio, Sandford, Dale, Saylor, Mike, Stover, Richard, Thompson, Matthew, Walp, Bernie, Ward, James, Wareham, John, Wei, Mingzhi, Wright, Chris
The Automated Planet Finder (APF) is a facility purpose-built for the discovery and characterization of extrasolar planets through high-cadence Doppler velocimetry of the reflex barycentric accelerations of their host stars. Located atop Mt. Hamilton
Externí odkaz:
http://arxiv.org/abs/1402.6684
Autor:
Lommen, Dave J. P., van Dishoeck, Ewine F., Wright, Chris M., Maddison, Sarah T., Min, Michiel, Wilner, David J., Salter, Demerese M., van Langevelde, Huib Jan, Bourke, Tyler L., van der Burg, Remco F. J., Blake, Geoffrey A.
Young stars are formed within dusty discs. The grains in the disc are originally of the same size as interstellar dust. Models predict that these grains will grow in size through coagulation. Observations of the silicate features at micron wavelength
Externí odkaz:
http://arxiv.org/abs/1004.0158
Autor:
Lommen, Dave, Maddison, Sarah, Wright, Chris, van Dishoeck, Ewine, Wilner, David, Bourke, Tyler
Grains in disks around young stars grow from interstellar submicron sizes to planetesimals over the course of several Myr. Thermal emission of large grains or pebbles can be best observed at cm wavelengths. However, other emission mechanisms can cont
Externí odkaz:
http://arxiv.org/abs/0812.3849