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搜索结果: 1-11 共查到天文学 c and d components相关记录11条 . 查询时间(0.093 秒)
The beaming effect (aka Doppler boosting) induces a variation in the observed flux of a luminous object, following its observed radial velocity variation. We describe a photometric signal induced by t...
We performed a statistical analysis of half-power pulse-widths of the core components in average pulsar profiles. We confirmed an existence of the lower bound of the distribution of half-power pulse-w...
We have selected a sample of 30 normal (non-cD) early type galaxies, for all of which optical spectroscopy is available, and which have been observed with Chandra to a depth such to insure the detecti...
1ES 1959+650 is one of the most remarkable high-peaked BL Lacertae objects (HBL). In 2002, it exhibited a TeV gamma-ray flare without a similar brightening of the synchrotron component at lower energi...
Activity in low-mass stars is an important ingredient in the evolution of such objects. Fundamental physical properties such as age, rotation, magnetic field are correlated with activity.
Orbital elements for bu 1240 ab. nature of the c and d components
Binaries with compact components:theoretical and Observational challenges
Ch cygni and other symbiotic stars with low luminosity Hot components
On the nature of the binary components of rxj0806.3+1527。
A new method to calculate simultaneosly both the unknown X and the components of the dispersion (results of measurement) is developed. An improved iterative algorihm is used.
The physical constraints were applied in the problem of deconvolution by explicitly correcting noise affected Fourier components of the unknown distribution. The method gives the constrained estimat...

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