Zobrazeno 1 - 10
of 200
pro vyhledávání: '"Cook, L M"'
Autor:
Henze, M., Darnley, M. J., Williams, S. C., Kato, M., Hachisu, I., Anupama, G. C., Arai, A., Boyd, D., Burke, D., Chinetti, K., Ciardullo, R., Cook, L. M., Cook, M. J., Erdman, P., Gao, X., Harris, B., Hartmann, D. H., Hornoch, K., Horst, J. Chuck, Hounsell, R., Husar, D., Itagaki, K., Kabashima, F., Kafka, S., Kaur, A., Kiyota, S., Kojiguchi, N., Kucakova, H., Kuramoto, K., Maehara, H., Mantero, A., Masci, F. J., Matsumoto, K., Naito, H., Ness, J. -U., Nishiyama, K., Oksanen, A., Osborne, J. P., Page, K. L., Paunzen, E., Pavana, M., Pickard, R., Prieto-Arranz, J., Rodriguez-Gil, P., Sala, G., Sano, Y., Shafter, A. W., Sugiura, Y., Tan, H., Tordai, T., Vratil, J., Wagner, R. M., Watanabe, F., Williams, B. F., Bode, M. F., Bruno, A., Buchheim, B., Crawford, T., Goff, B., Hernanz, M., Igarashi, A. S., Jose, J., Motta, M., O'Brien, T. J., Oswalt, T., Poyner, G., Ribeiro, V. A. R. M., Sabo, R., Shara, M. M., Shears, J., Starkey, D., Starrfield, S., Woodward, C. E.
Since its discovery in 2008, the Andromeda galaxy nova M31N 2008-12a has been observed in eruption every single year. This unprecedented frequency indicates an extreme object, with a massive white dwarf and a high accretion rate, which is the most pr
Externí odkaz:
http://arxiv.org/abs/1803.00181
Autor:
Andronov, Ivan L., Andrych, K. D., Antoniuk, K. A., Baklanov, A. V., Beringer, P., Breus, V. V., Burwitz, V., Chinarova, L. L., Chochol, D., Cook, L. M., Cook, M., Dubovský, P., Godłowski, W., Hegedüs, T., Hoňková, K., Hric, L., Jeon, Young-Beom, Juryšek, J., Kim, Chun-Hwey, Kim, Yonggi, Kim, Young-Hee, Kolesnikov, S. V., Kudashkina, L. S., Kusakin, A. V., Marsakova, V. I., Mason, P. A., Mašek, M., Mishevskiy, N., Nelson, R. H., Oksanen, A., Parimucha, S., Park, Ji-Won, Petrík, K., Quiñones, C., Reinsch, K., Robertson, J. W., Sergey, I. M., Szpanko, M., Tkachenko, M. G., Tkachuk, L. G., Traulsen, I., Tremko, J., Tsehmeystrenko, V. S., Yoon, Joh-Na, Zoła, S., Shakhovskoy, N. M.
The types of instability in the interacting binary stars are reviewed. The project "Inter-Longitude Astronomy" is a series of smaller projects on concrete stars or groups of stars. It has no special funds, and is supported from resources and grants o
Externí odkaz:
http://arxiv.org/abs/1702.02011
Autor:
Boyd, D. R. S., de Miguel, E., Patterson, J., Wood, M. A., Barrett, D., Boardman, J., Brettman, O., Cejudo, D., Collins, D., Cook, L. M., Cook, M. J., Foote, J. L., Fried, R., Gomez, T. L., Hambsch, F. -J., Jones, J. L., Kemp, J., Koff, R., Koppelman, M., Krajci, T., Lemay, D., Martin, B., McClusky, J. V., Menzies, K., Messier, D., Roberts, G., Robertson, J., Rock, J., Sabo, R., Skillman, D., Ulowetz, J., Vanmunster, T.
We present an analysis of photometric observations of the eclipsing novalike variable DW UMa made by the CBA consortium between 1999 and 2015. Analysis of 372 new and 260 previously published eclipse timings reveals a 13.6 year period or quasi-period
Externí odkaz:
http://arxiv.org/abs/1612.06883
Autor:
de Miguel, E., Patterson, J., Cejudo, D., Ulowetz, J., Jones, J. L., Boardman, J., Barret, D., Koff, R., Stein, W., Campbell, T., Vanmunster, T., Menzies, K., Slauson, D., Goff, W., Roberts, G., Morelle, E., Dvorak, S., Hambsch, F. -J., Starkey, D., Collins, D., Costello, M., Cook, M. J., Oksanen, A., Lemay, D., Cook, L. M., Ogmen, Y., Richmond, M., Kemp, J.
We report the results of a long campaign of time-series photometry on the nova-like variable UX Ursae Majoris during 2015. It spanned 150 nights, with ~1800 hours of coverage on 121 separate nights. The star was in its normal `high state' near magnit
Externí odkaz:
http://arxiv.org/abs/1512.08687
We report extensive photometry of the frequently outbursting dwarf nova RZ Leo Minoris. During two seasons of observations we detected 12 superoutbursts and 7 normal outbursts. The V magnitude of the star varied in range from 16.5 to 13.9 mag. The su
Externí odkaz:
http://arxiv.org/abs/0806.1657
We report extensive photometry of the dwarf nova V660 Herculis. During our campaign, lasting from August 2003 to November 2004, we recorded one bright eruption which turned out to be a superoutburst lasting about 15 days and having amplitude of ~4.5
Externí odkaz:
http://arxiv.org/abs/astro-ph/0506487
Autor:
Olech, A., Cook, L. M., Zloczewski, K., Mularczyk, K., Kedzierski, P., Udalski, A., Wisniewski, M.
We report extensive multi-station photometry of TT Boo during its June 2004 superoutburst. The amplitude of the superoutburst was about 5.5 mag and its length over 22 days. The star showed a small re-brightening starting around the 9th day of the sup
Externí odkaz:
http://arxiv.org/abs/astro-ph/0408080
Autor:
Nogami, D., Uemura, M., Ishioka, R., Iwamatsu, H., Kato, T., Pavlenko, E. P., Baklanov, A., Novak, R., Kiyota, S., Tanabe, K., Masi, G., Cook, L. M., Morikawa, K., Schmeer, P.
We report on the results of the QW Ser campaign which has been continued from 2000 to 2003 by the VSNET collaboration team. Four long outbursts and many short ones were caught during this period. Our intensive photometric observations revealed superh
Externí odkaz:
http://arxiv.org/abs/astro-ph/0310274
Autor:
Ishioka, R., Kato, T., Uemura, M., Pietz, J., Vanmunster, T., Krajci, T., Torii, K., Tanabe, K., Kiyota, S., Kinugasa, K., Masi, G., Morikawa, K., Cook, L. M., Schmeer, P., Yamaoka, H.
After 10 years of quiescence, HV Vir underwent a superoutburst in January 2002. We report time-series observations clearly revealing the period change of ordinary superhumps during the superoutburst. We derived a mean superhump period of 0.058260 d a
Externí odkaz:
http://arxiv.org/abs/astro-ph/0303224
Autor:
Nogami, D., Uemura, M., Ishioka, R., Kato, T., Torii, K., Starkey, D. R., Tanabe, K., Vanmunster, T., Pavlenko, E. P., Goranskij, V. P., Barsukova, E. A., Antoniuk, O., Martin, B., Cook, L. M., Masi, G., Mallia, F.
Publikováno v:
Astron.Astrophys. 404 (2003) 1067-1076
An intensive photometric-observation campaign of the recently discovered SU UMa-type dwarf nova, Var73 Dra was conducted from 2002 August to 2003 February. We caught three superoutbursts in 2002 October, December and 2003 February. The recurrence cyc
Externí odkaz:
http://arxiv.org/abs/astro-ph/0302538