Zobrazeno 1 - 10
of 3 712
pro vyhledávání: '"Kuhn, R"'
Autor:
Kenworthy, M. A., Mellon, S. N., Bailey III, J. I., Stuik, R., Dorval, P., Talens, G. -J. J., Crawford, S. R., Mamajek, E. E., Laginja, I., Ireland, M., Lomberg, B., Kuhn, R. B., Snellen, I., Zwintz, K., Kuschnig, R., Kennedy, G. M., Abe, L., Agabi, A., Mekarnia, D., Guillot, T., Schmider, F., Stee, P., de Pra, Y., Buttu, M., Crouzet, N., Kalas, P., Wang, J. J., Stevenson, K., de Mooij, E., Lagrange, A. -M., Lacour, S., Etangs, A. Lecavelier des, Nowak, M., Strøm, P. A., Hui, Z., Wang, L.
Publikováno v:
A&A 648, A15 (2021)
Photometric monitoring of Beta Pictoris in 1981 showed anomalous fluctuations of up to 4% over several days, consistent with foreground material transiting the stellar disk. The subsequent discovery of the gas giant planet Beta Pictoris b and the pre
Externí odkaz:
http://arxiv.org/abs/2102.05672
Autor:
Segura, N. Castro, Knigge, C., Acosta-Pulido, J. A., Altamirano, D., del Palacio, S., Santisteban, J. V. Hernandez, Pahari, M., Rodriguez-Gil, P., Belardi, C., Buckley, D. A. H., Burleigh, M. R., Childress, M., Fender, R. P., Hewitt, D. M., James, D. J., Kuhn, R. B., Kuin, N. P. M., Pepper, J., Ponomareva, A. A., Pretorius, M. L., Rodríguez, J. E., Stassun, K. G., Williams, D. R. A., Woudt, P. A.
V341 Ara was recently recognised as one of the closest (d ~ 150 pc) and brightest (V~ 10) nova-like cataclysmic variables. This unique system is surrounded by a bright emission nebula, likely to be the remnant of a recent nova eruption. Embedded with
Externí odkaz:
http://arxiv.org/abs/2008.07462
Autor:
Zwintz, K., Reese, D. R., Neiner, C., Pigulski, A., Kuschnig, R., Muellner, M., Zieba, S., Abe, L., Guillot, T., Handler, G., Kenworthy, M., Stuik, R., Moffat, A. F. J., Popowicz, A., Rucinski, S. M., Wade, G. A., Weiss, W. W., Bailey III, J. I., Crawford, S., Ireland, M., Kuhn, R., Lomberg, B., Mamajek, E. E., Mellon, S. N., Talens, G. J.
Publikováno v:
A&A 627, A28 (2019)
Exoplanet properties crucially depend on their host stars' parameters. In case the exoplanet host star shows pulsations, asteroseismology can be used for an improved description of the stellar parameters. We aim to revisit the pulsational properties
Externí odkaz:
http://arxiv.org/abs/1905.12545
Autor:
Dorval, P., Talens, G. J. J., Otten, G. P. P. L., Brahm, R., Jordán, A., Vanzi, L., Zapata, A., Henry, T., Paredes, L., Jao, W. C., James, H., Hinojosa, R., Bakos, G. A., Csubry, Z., Bhatti, W., Suc, V., Osip, D., Mamajek, E. E., Mellon, S. N., Wyttenbach, A., Stuik, R., Kenworthy, M., Bailey, J., Ireland, M., Crawford, S., Lomberg, B., Kuhn, R., Snellen, I.
Publikováno v:
A&A 635, A60 (2020)
In this paper, we aim to characterize a transiting planetary candidate in the southern skies found in the combined MASCARA and bRing data sets of HD 85628, an A3V star of V = 8.2 mag at a distance 172 pc, to confirm its planetary nature. The candidat
Externí odkaz:
http://arxiv.org/abs/1904.02733
Akademický článek
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Autor:
Vajda, F.J.E., O'Brien, T.J., Graham, J.E., Hitchcock, A.A., Perucca, P., Kuhn, R., Lander, C.M., Eadie, M.J.
Publikováno v:
In Epilepsy & Behavior July 2022 132
Autor:
Osborn, H. P., Rodriguez, J. E., Kenworthy, M. A., Kennedy, G. M., Mamajek, E. E., Robinson, C. E., Espaillat, C. C., Armstrong, D. J., Shappee, B. J., Bieryla, A., Latham, D. W., Anderson, D. R., Beatty, T. G., Berlind, P., Calkins, M. L., Esquerdo, G. A., Gaudi, B. S., Hellier, C., Holoien, T. W. -S., James, D., Kochanek, C. S., Kuhn, R. B., Lund, M. B., Pepper, J., Pollacco, D. L., Prieto, J. L., Siverd, R. J., Stassun, K. G., Stevens, D. J., Stanek, K. Z., West, R. G.
We report the discovery of eclipses by circumstellar disc material associated with the young star PDS 110 in the Ori OB1a association using the SuperWASP and KELT surveys. PDS 110 (HD 290380, IRAS 05209-0107) is a rare Fe/Ge-type star, a ~10 Myr-old
Externí odkaz:
http://arxiv.org/abs/1705.10346
Autor:
Temple, L. Y., Hellier, C., Albrow, M. D., Anderson, D. R., Bayliss, D., Beatty, T. G., Bieryla, A., Brown, D. J. A., Cargile, P. A., Cameron, A. Collier, Collins, K. A., Colón, K. D., Curtis, I. A., D'Ago, G., Delrez, L., Eastman, J., Gaudi, B. S., Gillon, M., Gregorio, J., James, D., Jehin, E., Joner, M. D., Kielkopf, J. F., Kuhn, R. B., Labadie-Bartz, J., Latham, D. W., Lendl, M., Lund, M. B., Malpas, A. L., Maxted, P. F. L., Myers, G., Oberst, T. E., Pepe, F., Pepper, J., Pollacco, D., Queloz, D., Rodriguez, J. E., Ségransan, D., Siverd, R. J., Smalley, B., Stassun, K. G., Stevens, D. J., Stockdale, C., Tan, T. G., Triaud, A. H. M. J., Udry, S., Villanueva Jr, S., West, R. G., Zhou, G.
We report the joint WASP/KELT discovery of WASP-167b/KELT-13b, a transiting hot Jupiter with a 2.02-d orbit around a $V$ = 10.5, F1V star with [Fe/H] = 0.1 $\pm$ 0.1. The 1.5 R$_{\rm Jup}$ planet was confirmed by Doppler tomography of the stellar lin
Externí odkaz:
http://arxiv.org/abs/1704.07771