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911.
Essential macroscopic internal properties of compact objects can be related to each other with the help of General Relativity.
A somewhat familiar example is the relationship between the compactness M/R and the gravitational redshift for nonrotating bodies. Rotation poses new challenges when trying to relate observed or potentially
observed quantities such as the graviational redshift, mass, radius, and angular velocity. Using a perturbative approach,
we present an analytical approximation whose purpose is to relate these quantities. Two main results are highlighted: Derivation
of a new maximal angular velocity depending only on the mass of the object and a possible estimate of the radius from a measurement
of the gravitational redshift. 相似文献
912.
Jianpo Guo Fenghui Zhang Xianfei Zhang Zhanwen Han 《Astrophysics and Space Science》2010,325(1):25-30
Ultraviolet radiation is a double-edged sword to life. If it is too strong, the terrestrial biological systems will be damaged.
And if it is too weak, the synthesis of many biochemical compounds cannot go along. We try to obtain the continuous ultraviolet
habitable zones, and compare the ultraviolet habitable zones with the habitable zones of host stars. Using the boundary ultraviolet
radiation of ultraviolet habitable zone, we calculate the ultraviolet habitable zones of host stars with masses from 0.08
to 4.00 M
⊙. For the host stars with effective temperatures lower than 4,600 K, the ultraviolet habitable zones are closer than the habitable
zones. For the host stars with effective temperatures higher than 7,137 K, the ultraviolet habitable zones are farther than
the habitable zones. For a hot subdwarf as a host star, the distance of the ultraviolet habitable zone is about ten times
more than that of the habitable zone, which is not suitable for the existence of life. 相似文献
913.
Evaluation of the intermediate-term periodicities in solar and cosmic ray activities during cycle 23
In this paper we investigate the presence and temporal evolution of galactic cosmic rays (GCRs) time-series and three solar
parameters, namely the daily sunspot number, the coronal green line and the 10.7 cm solar radio flux over the period 1996–2003
by the wavelet technique. A number of short- and intermediate-term quasi-periodicities were also detected in both GCR and
solar parameters. For the short-term range, we have identified quasi-periods of 16–30 days, 40–55 days, 60–70 days, 80–90 days
and 80–100 days. In the case of intermediate range, the significant periods were 120–140 days, 150–170 days, 190–210 days,
240–260 days, ≈1.09 yr. and ≈1.23 yr. The wavelet power spectra show that all the above-mentioned periods are intermittent
in nature and occurred in different time-series in different intervals. The result exhibits that the well-known “Rieger period”
of (150–160 days) was prominent in both GCR and solar data sets during the ascending phase of cycle 23. Possible reasons behind
the observed periods were discussed with the help of previous results and existing numerical models. 相似文献
914.
Pascal Chardonnet Valery Chechetkin Lev Titarchuk 《Astrophysics and Space Science》2010,325(2):153-161
We present a model of a gamma-ray burst (GRB) related to “very massive” stars. In the framework of our model, the GRB phenomenon
is a result of helium burning in degenerate conditions in a massive star (≳130 M
⊙), in which the thermal nuclear burning occurs in the deflagration regime and has a pulsating temporal pattern. The shock
runs away from the burning (reaction) zone, which leads to the development of a coronal outflow (jet-like) structure. In our
scenario the GRB observable prompt fast rise and decay part can be a result of photon propagation through the hot corona (Comptonization
photosphere) of the star. On the other hand, the GRB afterglow is a cooling phase of the expanding and outflowing envelope.
Presumably, the X-ray part of the GRB emergent spectrum is formed due to upscattering of soft photons of outer layers of the
star off hot coronal electrons, and thus it should have a specific shape of the Comptonization spectrum. 相似文献
915.
Nikolay A. Sokolov 《Astrophysics and Space Science》2010,325(1):37-40
We presented a phenomenological mode that attributes the precession of perihelion of planets to the relativistic correction.
This modifies Newton’s equation by adding an inversely cube term with distance. The total energy of the new system is found
to be the same as the Newtonian one. Moreover, we have deduced the deflection of light formula from Rutherford scattering.
The relativistic term can be accounted for quantum correction of the gravitational potential and/or self energy of objects. 相似文献
916.
To investigate the dependence of the Holmberg effect of paired galaxies on three-dimensional separations, we have constructed
four subsamples characterized by three-dimensional separations s ≤ 50 kpc, 50 kpc < s ≤ 100 kpc , 100kpc < s ≤150kpc , and
150 kpc < s ≤ 200 kpc , respectively. In this study, linear correlation coefficients and surplus standard deviations of color
indices, luminosity, and size between two components of paired galaxies are calculated. It is found that there is a weak tendency
for correlation coefficients of color indices to increase with decreasing three-dimensional separations, but such a tendency
does not exist for ones of luminosity and size. We also note that there is no tendency for surplus standard deviations to
decrease with decreasing three-dimensional separations. This suggests that it is still very difficult to clearly affirm the
dependence of the Holmberg Effect of paired galaxies on three-dimensional separations. 相似文献
917.
Jayanta Roy Yashwant Gupta Ue-Li Pen Jeffrey B. Peterson Sanjay Kudale Jitendra Kodilkar 《Experimental Astronomy》2010,28(1):25-60
The new era of software signal processing has a large impact on radio astronomy instrumentation. Our design and implementation
of a 32 antennae, 33 MHz, dual polarization, fully real-time software backend for the GMRT, using only off-the-shelf components,
is an example of this. We have built a correlator and a beamformer, using PCI-based ADC cards and a Linux cluster of 48 nodes
with dual gigabit inter-node connectivity for real-time data transfer requirements. The highly optimized compute pipeline
uses cache efficient, multi-threaded parallel code, with the aid of vectorized processing. This backend allows flexibility
in final time and frequency resolutions, and the ability to implement algorithms for radio frequency interference rejection.
Our approach has allowed relatively rapid development of a fairly sophisticated and flexible backend receiver system for the
GMRT, which will greatly enhance the productivity of the telescope. In this paper we describe some of the first lights using
this software processing pipeline. We believe this is the first instance of such a real-time observatory backend for an intermediate
sized array like the GMRT. 相似文献
918.
Nonlinear electron-acoustic solitary waves (EASWs) are studied using Sagdeev’s pseudo-potential technique in a collisionless
unmagnetized plasma consisting of a cold electron fluid, nonthermal hot electrons and stationary ions. It is shown that the
presence of fast nonthermal electrons may modify the parametric region where electron-acoustic solitons may exist. Our investigation
is of wide relevance to astronomers and space scientists working on interstellar space plasmas. 相似文献
919.
Murli Manohar Verma 《Astrophysics and Space Science》2010,330(1):101-105
We propose a time-varying cosmological constant with a fixed equation of state, which evolves mainly through its interaction
with the background during most of the long history of the universe. However, such an interaction does not exist in the very
early- and the late-time universe and this produces the acceleration during these eras when it becomes very nearly a constant.
It is found that after the initial inflationary phase, the cosmological constant, which we call the lambda parameter, rolls
down from a large constant value to another but very small constant value and further dominates the present epoch showing
up in the form of dark energy, driving the acceleration. 相似文献
920.
The use of invariant manifolds for transfers between unstable periodic orbits of different energies 总被引:1,自引:0,他引:1
Kathryn E. Davis Rodney L. Anderson Daniel J. Scheeres George H. Born 《Celestial Mechanics and Dynamical Astronomy》2010,107(4):471-485
Techniques from dynamical systems theory have been applied to the construction of transfers between unstable periodic orbits
that have different energies. Invariant manifolds, trajectories that asymptotically depart or approach unstable periodic orbits,
are used to connect the initial and final orbits. The transfer asymptotically departs the initial orbit on a trajectory contained
within the initial orbit’s unstable manifold and later asymptotically approaches the final orbit on a trajectory contained
within the stable manifold of the final orbit. The manifold trajectories are connected by the execution of impulsive maneuvers.
Two-body parameters dictate the selection of the individual manifold trajectories used to construct efficient transfers. A
bounding sphere centered on the secondary, with a radius less than the sphere of influence of the secondary, is used to study
the manifold trajectories. A two-body parameter, κ, is computed within the bounding sphere, where the gravitational effects of the secondary dominate. The parameter κ is defined as the sum of two quantities: the difference in the normalized angular momentum vectors and eccentricity vectors
between a point on the unstable manifold and a point on the stable manifold. It is numerically demonstrated that as the κ parameter decreases, the total cost to complete the transfer decreases. Preliminary results indicate that this method of
constructing transfers produces a significant cost savings over methods that do not employ the use of invariant manifolds. 相似文献