Zobrazeno 1 - 10
of 378
pro vyhledávání: '"Linsky, Jeffrey L."'
Autor:
Herczeg, Gregory J., Chen, Yuguang, Donati, Jean-Francois, Dupree, Andrea K., Walter, Frederick M., Hillenbrand, Lynne A., Johns-Krull, Christopher M., Manara, Carlo F., Guenther, Hans Moritz, Fang, Min, Schneider, P. Christian, Valenti, Jeff A., Alencar, Silvia H. P., Venuti, Laura, Alcala, Juan Manuel, Frasca, Antonio, Arulanantham, Nicole, Linsky, Jeffrey L., Bouvier, Jerome, Brickhouse, Nancy S., Calvet, Nuria, Espaillat, Catherine C., Campbell-White, Justyn, Carpenter, John M., Chang, Seok-Jun, Cruz, Kelle L., Dahm, S. E., Eisloeffel, Jochen, Edwards, Suzan, Fischer, William J., Guo, Zhen, Henning, Thomas, Ji, Tao, Jose, Jesse, Kastner, Joel H., Launhardt, Ralf, Principe, David A., Robinson, Conner E., Serna, Javier, Siwak, Michal, Sterzik, Michael F., Takasao, Shinsuke
Accretion plays a central role in the physics that governs the evolution and dispersal of protoplanetary disks. The primary goal of this paper is to analyze the stability over time of the mass accretion rate onto TW Hya, the nearest accreting solar-m
Externí odkaz:
http://arxiv.org/abs/2308.14590
Autor:
Sterken, Veerle J., Hunziker, Silvan, Dialynas, Kostas, Leitner, Jan, Sommer, Maximilian, Srama, Ralf, Baalmann, Lennart R., Li, Aigen, Herbst, Konstantin, Galli, André, Brandt, Pontus, Riebe, My, Baggaley, Jack, Blanc, Michel, Czechowski, Andrej, Effenberger, Frederic, Fields, Brian, Frisch, Priscilla, Horanyi, Mihaly, Hsu, Hsiang-Wen, Khawaja, Nozair, Krüger, Harald, Kurth, Bill S., Ligterink, Niels F. W., Linsky, Jeffrey L., Lisse, Casey, Malaspina, David, Miller, Jesse A., Opher, Merav, Poppe, Andrew R., Postberg, Frank, Provornikova, Elena, Redfield, Seth, Richardson, John, Rowan-Robinson, Michael, Scherer, Klaus, Shen, Mitchell M., Slavin, Jon D., Sternovsky, Zoltan, Stober, Gunter, Strub, Peter, Szalay, Jamey, Trieloff, Mario
Publikováno v:
RAS Techniques and Instruments, rzad034 (2023)
We discuss the synergies between heliospheric and dust science, the open science questions, the technological endeavors and programmatic aspects that are important to maintain or develop in the decade to come. In particular, we illustrate how we can
Externí odkaz:
http://arxiv.org/abs/2308.10728
Autor:
Linsky, Jeffrey L., Moebius, Eberhard
The Voyager spacecraft are providing the first in situ measurements of physical properties in the outer heliosphere beyond the heliopause. These data, together with data from the IBEX and HST spacecraft and physical models consistent with these data,
Externí odkaz:
http://arxiv.org/abs/2212.00777
Autor:
Swaczyna, Paweł, Schwadron, Nathan A., Möbius, Eberhard, Bzowski, Maciej, Frisch, Priscilla C., Linsky, Jeffrey L., McComas, David J., Rahmanifard, Fatemeh, Redfield, Seth, Winslow, Réka M., Wood, Brian E., Zank, Gary P.
Publikováno v:
ApJL, 937 (2022), L32
On its journey through the Galaxy, the Sun passes through diverse regions of the interstellar medium. High-resolution spectroscopic measurements of interstellar absorption lines in spectra of nearby stars show absorption components from more than a d
Externí odkaz:
http://arxiv.org/abs/2209.09927
Analysis of interstellar absorption lines observed in high-resolution {\em HST} spectra of nearby stars provides temperatures, turbulent velocities, and kinetic properties of warm interstellar clouds. Previous studies identified 15 warm partially ion
Externí odkaz:
http://arxiv.org/abs/2204.02428
Autor:
Youngblood, Allison, Pineda, J. Sebastian, Ayres, Thomas, France, Kevin, Linsky, Jeffrey L., Wood, Brian E., Redfield, Seth, Schlieder, Joshua E.
Observations of H I Lyman alpha, the brightest UV emission line of late-type stars, are critical for understanding stellar chromospheres and transition regions, modeling photochemistry in exoplanet atmospheres, and measuring the abundances of neutral
Externí odkaz:
http://arxiv.org/abs/2201.01315
Autor:
Wood, Brian E., Mueller, Hans-Reinhard, Redfield, Seth, Konow, Fallon, Vannier, Hunter, Linsky, Jeffrey L., Youngblood, Allison, Vidotto, Aline A., Jardine, Moira, Alvarado-Gomez, Julian D., Drake, Jeremy J.
High resolution UV spectra of stellar H I Lyman-alpha lines from the Hubble Space Telescope (HST) provide observational constraints on the winds of coronal main sequence stars, thanks to an astrospheric absorption signature created by the interaction
Externí odkaz:
http://arxiv.org/abs/2105.00019
Autor:
Carleo, Ilaria, Youngblood, Allison, Redfield, Seth, Barris, Nuria Casasayas, Ayres, Thomas R., Vannier, Hunter, Fossati, Luca, Palle, Enric, Livingston, John H., Lanza, Antonino F., Niraula, Prajwal, Alvarado-Gómez, Julián D., Chen, Guo, Gandolfi, Davide, Guenther, Eike W., Linsky, Jeffrey L., Nagel, Evangelos, Narita, Norio, Nortmann, Lisa, Shkolnik, Evgenya L., Stangret, Monika
GJ9827 is a bright star hosting a planetary system with three transiting planets. As a multi-planet system with planets that sprawl within the boundaries of the radius gap between terrestrial and gaseous planets, GJ9827 is an optimal target to study
Externí odkaz:
http://arxiv.org/abs/2101.06277
Stellar ultraviolet (UV) radiation drives photochemistry, and extreme-ultraviolet (EUV) radiation drives mass loss in exoplanet atmospheres. However, the UV flux is partly unobservable due to interstellar absorption, particularly in the EUV range (10
Externí odkaz:
http://arxiv.org/abs/2012.11738
Autor:
Melbourne, Katherine, Youngblood, Allison, France, Kevin, Froning, C. S., Pineda, J. Sebastian, Shkolnik, Evgenya L., Wilson, David J., Wood, Brian E., Basu, Sarbani, Roberge, Aki, Schlieder, Joshua E., Cauley, P. Wilson, Loyd, R. O. Parke, Newton, Elisabeth R., Schneider, Adam, Arulanantham, Nicole, Berta-Thompson, Zachory, Brown, Alexander, Buccino, Andrea P., Kempton, Eliza, Linsky, Jeffrey L., Logsdon, Sarah E., Mauas, Pablo, Pagano, Isabella, Peacock, Sarah, Redfield, Seth, Rugheimer, Sarah, Schneider, P. Christian, Teal, D. J., Tian, Feng, Tilipman, Dennis, Vieytes, Mariela
M dwarf stars are excellent candidates around which to search for exoplanets, including temperate, Earth-sized planets. To evaluate the photochemistry of the planetary atmosphere, it is essential to characterize the UV spectral energy distribution of
Externí odkaz:
http://arxiv.org/abs/2009.07869