Results 61 to 70 of about 8,054,126 (389)
Predicting Variable Star Light Curves [PDF]
International Astronomical Union Colloquium, 1993 AbstractI present a new method to test determinism, in particular the nonlinear behavior, in observed time series of pulsating stars, based on a recent prediction method which exploits the dynamical system theory. A method for filling gaps in data has thereby been constructed.
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Light on curved backgrounds [PDF]
Physical Review D, 2015 34 pages, 10 ...
Batic, D., Nelson, S., Nowakowski, M.
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The radial pulsation of AI Aurigae [PDF]
, 2001 We present an analysis of eleven years of Stromgren by photometry of the red semiregular variable star AI Aurigae. An early period determination of 63.9 days is confirmed by the long-term light curve behaviour.
Alvarez +37 more
core +2 more sources
The Optical Variability of Supermassive Black Hole Binary Candidate PG 1302–102: Periodicity and Perturbation in the Light Curve [PDF]
Astrophysical Journal, 2018 The photometric light curve of PG 1302–102 shows periodic variability, which makes this object one of the most plausible supermassive black hole binary candidates. Interestingly, the most recent study of its updated optical light curve reports a decrease
A. Kovačević +3 more
semanticscholar +1 more source
Swift/BAT and RXTE Observations of the Peculiar X-ray Binary 4U 2206+54 - Disappearance of the 9.6 Day Modulation [PDF]
, 2006 Observations of the high-mass X-ray binary 4U 2206+54 with the Swift Burst Alert Telescope (BAT) do not show modulation at the previously reported period of 9.6 days found from observations made with the Rossi X-ray Timing Explorer (RXTE) All-Sky Monitor
Corbet, R. H. D. +2 more
core +4 more sources
The bumpy light curve of Type IIn supernova iPTF13z over 3 years [PDF]
, 2017 Author(s): Nyholm, A; Sollerman, J; Taddia, F; Fremling, C; Moriya, TJ; Ofek, EO; Gal-Yam, A; De Cia, A; Roy, R; Kasliwal, MM; Cao, Y; Nugent, PE; Masci, FJ | Abstract: ©2017 ESO.
A. Nyholm +12 more
semanticscholar +1 more source
The late-time light curve of the type Ia supernova SN 2011fe [PDF]
, 2017 We present late-time optical R-band imaging data from the Palomar Transient Factory (PTF) for the nearby Type Ia supernova SN 2011fe. The stacked PTF light curve provides densely sampled coverage down to R ≃ 22 mag over 200–620 d past explosion ...
G. Dimitriadis +12 more
semanticscholar +1 more source
VBBinaryLensing: a public package for microlensing light-curve computation [PDF]
Monthly notices of the Royal Astronomical Society, 2018 The computation of microlensing light curves represents a bottleneck for the modeling of planetary events, making broad searches in the vast parameter space of microlensing extremely time-consuming.
V. Bozza +6 more
semanticscholar +1 more source
Tycho Brahe's supernova: light from centuries past [PDF]
, 2003 The light curve of SN 1572 is described in the terms used nowadays to characterize SNeIa. By assembling the records of the observations done in 1572--74 and evaluating their uncertainties, it is possible to recover the light curve and the color evolution
Albinson J. S. +6 more
core +1 more source
, 2013 Presented at the "40 Years of Variable Stars: A Celebration of Contributions by Horace A. Smith" conference (arXiv:1310.0149).
Molnar, Lawrence +2 more
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