Zobrazeno 1 - 10
of 388
pro vyhledávání: '"Templeton M."'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
Russell, T. D., Miller-Jones, J. C. A., Sivakoff, G. R., Altamirano, D., O'Brien, T. J., Page, K. L., Templeton, M. R., Koerding, E. G., Knigge, C., Rupen, M. P., Fender, R. P., Heinz, S., Maitra, D., Markoff, S., Migliari, S., Remillard, R. A., Russell, D. M., Sarazin, C. L., Waagen, E. O.
We present the results of our intensive radio observing campaign of the dwarf nova SS Cyg during its 2010 April outburst. We argue that the observed radio emission was produced by synchrotron emission from a transient radio jet. Comparing the radio l
Externí odkaz:
http://arxiv.org/abs/1605.07136
The semi-regular variable star RU Vulpeculae (RU Vul) is being observed visually since 1935. Its pulsation period and amplitude are declining since $\sim1954$. A leading hypothesis to explain the period decrease in asymptotic giant branch (AGB) stars
Externí odkaz:
http://arxiv.org/abs/1511.03224
Autor:
Munari, U., Henden, A., Frigo, A., Zwitter, T., Bienayme, O., Bland-Hawthorn, J., Boeche, C., Freeman, K. C., Gilmore, G., Gibson, B. K., Grebel, E. K., Helmi, A., Kordopatis, G., Levine, S. E., Navarro, J. F., Parker, Q. A., Reid, W., Seabroke, G. M., Siebert, A., Siviero, A., Smith, T. C., Steinmetz, M., Templeton, M., Terrell, D., Welch, D. L., Williams, M., Wyse, R. F. G.
We provide APASS photometry in the Landolt BV and Sloan g'r'i' bands for all the 425,743 stars included in the latest 4th RAVE Data Release. The internal accuracy of the APASS photometry of RAVE stars, expressed as error of the mean of data obtained
Externí odkaz:
http://arxiv.org/abs/1408.5476
Autor:
Miller-Jones, J. C. A., Sivakoff, G. R., Knigge, C., Körding, E. G., Templeton, M., Waagen, E. O.
Publikováno v:
Science, 24 May 2013, Vol. 340, No. 6135, pp. 950-952
Dwarf novae are white dwarfs accreting matter from a nearby red dwarf companion. Their regular outbursts are explained by a thermal-viscous instability in the accretion disc, described by the disc instability model that has since been successfully ex
Externí odkaz:
http://arxiv.org/abs/1305.5846
Autor:
Templeton, M., Henden, A., Goff, W., Smith, S., Sabo, R., Walker, G., Buchheim, R., Belcheva, G., Crawford, T., Cook, M., Dvorak, S., Harris, B.
We present a modern ephemeris and modern light curve of the first-discovered Cepheid variable in M31, Edwin Hubble's M31-V1. Observers of the American Association of Variable Star Observers undertook these observations during the latter half of 2010.
Externí odkaz:
http://arxiv.org/abs/1111.0262
High spatial resolution observations of the H\alpha-emitting wind structure associated with the Luminous Blue Variable star P Cygni were obtained with the Navy Prototype Optical Interferometer (NPOI). These observations represent the most comprehensi
Externí odkaz:
http://arxiv.org/abs/1004.0376
We present the results of a two-year, multisite observing campaign investigating the high-amplitude delta Scuti star VX Hydrae during the 2006 and 2007 observing seasons. The final data set consists of nearly 8500 V-band observations spanning HJD 245
Externí odkaz:
http://arxiv.org/abs/0909.5409
Autor:
Templeton, M. R., Henden, A. A.
Publikováno v:
Astron.J.134:1999-2005,2007
We present the results of recent long-term BVRcIc photometric monitoring of the type II Cepheid prototype W Virginis. These new observations, made during the 2006 and 2007 observing season, represent the longest homogeneous, multicolor light curve of
Externí odkaz:
http://arxiv.org/abs/0709.0401
Autor:
Templeton, M. R., Leaman, R., Szkody, P., Henden, A., Cook, L., Starkey, D., Oksanen, A., Koppelman, M., Boyd, D., Nelson, P. R., Vanmunster, T., Pickard, R., Quinn, N., Huziak, R., Aho, M., James, R., Golovin, A., Pavlenko, E., Durkee, R. I., Crawford, T. R., Walker, G., Paakkonen, P.
The cataclysmic variable ASAS J002511+1217.2 was discovered in outburst by the All-Sky Automated Survey in September 2004, and intensively monitored by AAVSO observers through the following two months. Both photometry and spectroscopy indicate that t
Externí odkaz:
http://arxiv.org/abs/astro-ph/0510078