Zobrazeno 1 - 10
of 211
pro vyhledávání: '"Linsky J"'
Autor:
Airapetian, V. S., Adibekyan, V., Ansdell, M., Alexander, D., Bastian, T., Saikia, S. Boro, Brun, A. S., Cohen, O., Cuntz, M., Danchi, W., Davenport, J., DeNolfo, J., DeVore, R., Dong, C. F., Drake, J. J., France, K., Fraschetti, F., Herbst, K., Garcia-Sage, K., Gillon, M., Glocer, A., Grenfell, J. L., Gronoff, G., Gopalswamy, N., Guedel, M., Hartnett, H., Harutyunyan, H., Hinkel, N. R., Jensen, A. G., Jin, M., Johnstone, C., Kalas, P., Kane, S. R., Kay, C., Kitiashvili, I. N., Kochukhov, O., Kondrashov, D., Lazio, J., Leake, J., Li, G., Linsky, J., Lueftinger, T., Lynch, B., Lyra, W., Mandell, A. M., Mandt, K. E., Maehara, H., Miesch, M. S., Mickaelian, A. M., Mouchou, S., Notsu, Y., Ofman, L., Oman, L. D., Osten, R. A., Oran, R., Petre, R., Ramirez, R. M., Rau, G., Redfield, S., Réville, V., Rugheimer, S., Scheucher, M., Schlieder, J. E., Shibata, K., Schnittman, J. D., Soderblom, David, Strugarek, A., Turner, J. D., Usmanov, A., Der Holst, Van, Vidotto, A., Vourlidas, A., Way, M. J., Wolk, Zank, G. P., R., P. Zarka, Kopparapu, Babakhanova, S., Pevtsov, A. A., Lee, Y., Henning, W., Colón, K. D., Wolf, E. T.
The field of exoplanetary science is making rapid progress both in statistical studies of exoplanet properties as well as in individual characterization. As space missions provide an emerging picture of formation and evolution of exoplanetary systems
Externí odkaz:
http://arxiv.org/abs/1903.06853
Autor:
Froning, C. S., Kowalski, A., France, K., Loyd, R. O. Parke, Schneider, P. Christian, Youngblood, A., Wilson, D., Brown, A., Berta-Thompson, Z., Pineda, J. Sebastian, Linsky, J., Rugheimer, S., Miguel, Y.
As part of the Mega MUSCLES Hubble Space Telescope (HST) Treasury program, we obtained time-series ultraviolet spectroscopy of the M2.5V star, GJ~674. During the FUV monitoring observations, the target exhibited several small flares and one large fla
Externí odkaz:
http://arxiv.org/abs/1901.08647
Autor:
Brandt, Pontus C., Provornikova, E.A., Cocoros, A., Turner, D., DeMajistre, R., Runyon, K., Lisse, C.M., Bale, S., Kurth, W.S., Galli, A., Wurz, P., McNutt, Ralph L., Jr., Wimmer-Schweingruber, R., Linsky, J., Redfield, S., Kollmann, P., Mandt, K.E., Rymer, A.M., Roelof, E.C., Kinnison, J., Opher, M., Hill, M.E., Paul, M.V.
Publikováno v:
In Acta Astronautica October 2022 199:364-373
We model the atmospheres and spectra of Earth-like planets orbiting the entire grid of M dwarfs for active and inactive stellar models with $T_{eff}$ = 2300K to $T_{eff}$ = 3800K and for six observed MUSCLES M dwarfs with UV radiation data. We set th
Externí odkaz:
http://arxiv.org/abs/1506.07202
Autor:
Fossati, L., Bourrier, V., Ehrenreich, D., Haswell, C. A., Kislyakova, K. G., Lammer, H., Etangs, A. Lecavelier des, Alibert, Y., Ayres, T. R., Ballester, G. E., Barnes, J., Bisikalo, D. V., Collier, A., Cameron, Czesla, S., Desert, J. -M., France, K., Guedel, M., Guenther, E., Helling, Ch., Heng, K., Homstrom, M., Kaltenegger, L., Koskinen, T., Lanza, A. F., Linsky, J. L., Mordasini, C., Pagano, I., Pollacco, D., Rauer, H., Reiners, A., Salz, M., Schneider, P. C., Shematovich, V. I., Staab, D., Vidotto, A. A., Wheatley, P. J., Wood, B. E., Yelle, R. V.
Exoplanet science is now in its full expansion, particularly after the CoRoT and Kepler space missions that led us to the discovery of thousands of extra-solar planets. The last decade has taught us that UV observations play a major role in advancing
Externí odkaz:
http://arxiv.org/abs/1503.01278
Autor:
Cowan, N. B., Greene, T., Angerhausen, D., Batalha, N. E., Clampin, M., Colon, K., Crossfield, I. J. M., Fortney, J. J., Gaudi, B. S., Harrington, J., Iro, N., Lillie, C. F., Linsky, J. L., Lopez-Morales, M., Mandell, A. M., Stevenson, K. B.
[Abridged] We have only been able to comprehensively characterize the atmospheres of a handful of transiting planets, because most orbit faint stars. TESS will discover transiting planets orbiting the brightest stars, enabling, in principle, an atmos
Externí odkaz:
http://arxiv.org/abs/1502.00004
Autor:
Bailey, J. D., Grunhut, J., Shultz, M., Wade, G., Landstreet, J. D., Bohlender, D., Lim, J., Wong, K., Drake, S., Linsky, J., Collaboration, the MiMeS
HD 133880 is a rapidly rotating Bp star and host to one of the strongest magnetic fields of any Bp star. A member of the Upper Centaurus Lupus association, it is a star with a well-determined age of 16 Myr. Twelve new spectra obtained from the FEROS,
Externí odkaz:
http://arxiv.org/abs/1203.5277
Autor:
Herczeg, G. J., Walter, F. M., Linsky, J. L., Gahm, G. F., Ardila, D. R., Brown, A., Johns-Krull, C. M., Simon, M., Valenti, J. A.
We present far-ultraviolet spectra of the classical T Tauri star RU Lupi covering the 912-1710 A spectral range, as observed by the HST/STIS and FUSE satellites. We use these spectra, which are rich in emission and absorption lines, to probe both the
Externí odkaz:
http://arxiv.org/abs/astro-ph/0504654
Publikováno v:
Astrophys.J. 622 (2005) 629-652
FUSE ultraviolet spectra of 8 giant and supergiant stars reveal that high temperature (3 X 10^5 K) atmospheres are common in luminous cool stars and extend across the color-magnitude diagram from Alpha Car (F0 II) to the cool giant Alpha Tau (K5 III)
Externí odkaz:
http://arxiv.org/abs/astro-ph/0412539
Autor:
Osten, R. A., Brown, A., Ayres, T. R., Drake, S. A., Franciosini, E., Pallavicini, R., Tagliaferri, G., Stewart, R. T., Skinner, S. L., Linsky, J. L.
We report on four years of multiple wavelength observations of the RS CVn system V711 Tau (HR 1099) from 1993, 1994, 1996, and 1998. This combination of radio, ultraviolet, extreme ultraviolet, and X-ray observations allows us to view, in the most co
Externí odkaz:
http://arxiv.org/abs/astro-ph/0402613