中文
相关论文

相关论文: Secular Aberration Drift and IAU Definition of ICR…

200 篇论文

The centrifugial acceleration of the Solar system, resulting from the gravitational attraction of the Galaxy centre, causes a phenomenon known as 'secular aberrration drift'. This acceleration of the Solar system barycentre has been ignored…

天体物理仪器与方法 · 物理学 2013-11-06 Oleg Titov

The motion of the barycenter of the Solar System (SSB), the origin of the International Celestial Reference System, causes a directional displacement known as secular aberration. The secular aberration drift caused by the galactocentric…

天体物理仪器与方法 · 物理学 2024-07-30 Niu Liu , Zi Zhu , Jia-Cheng Liu

The galactocentric rotation of the Solar system generates the systematic effect in proper motions known as 'secular aberration drift'. This tiny effect (about five microseconds per year) in the quasar proper motion can be measured by VLBI.…

天体物理学 · 物理学 2008-05-09 O. Titov

One of the main endeavors of fundamental astrometry is to establish a practical realization of an inertial reference frame anchored to celestial objects whose positions are defined in the barycentric coordinates of the solar system. The…

天体物理学 · 物理学 2008-11-26 Sergei M. Kopeikin , Valeri V. Makarov

A recent paper demonstrated the existence of a secular aberration drift term in stellar proper motions that arises when transforming an astrometric catalogue defined for an observer at rest with respect to the solar system barycentre to…

天体物理仪器与方法 · 物理学 2025-03-26 Anthony G. A. Brown , Ulrich Bastian , Sergei Klioner

Extragalactic proper motions can reveal a variety of cosmological and local phenomena over a range of angular scales. These include observer-induced proper motions, such as the secular aberration drift caused by the solar acceleration about…

宇宙学与河外天体物理 · 物理学 2019-04-02 Jeremy Darling , Alexandra Truebenbach , Jennie Paine

During the last years, much attention has been paid to the astrometric implications of the galactic aberration in proper motions (GA). This effect causes systematic errors in astrometric measurements at a microarcsecond level. Some authors…

天体物理仪器与方法 · 物理学 2015-02-03 Zinovy Malkin

We propose new estimates of the secular aberration drift, mainly due to the rotation of the Solar System about the Galactic center, based on up-to-date VLBI observations and and improved method of outlier elimination. We fit degree-2 vector…

天体物理仪器与方法 · 物理学 2015-06-17 O. Titov , S. Lambert

Cosmic ray acceleration by shocks related with Slipping Interaction Regions (SIRs) in the Galactic Wind is considered. SIRs are similar to Solar Wind Corotating Interaction Regions. The spiral structure of our Galaxy results in a strong…

天体物理学 · 物理学 2009-11-10 H. J. Voelk , V. N. Zirakashvili

The secular perturbations exerted by an inclined satellite orbiting in a gap in a broad planetary ring tends to excite the inclinations of the nearby ring particles, and the ring's self-gravity can allow that disturbance to propagate away…

天体物理学 · 物理学 2009-11-13 J. M. Hahn

According to the Cosmological Principle an observer stationary with respect to the comoving coordinates of the expanding universe should find the redshift distribution of distant quasars to be isotropic. However, the observed redshift…

宇宙学与河外天体物理 · 物理学 2025-09-01 Ashok K. Singal

We propose an alternative method to detect the secular aberration drift induced by the solar system acceleration due to the attraction to the Galaxy centre. This method is free of the individual radio source proper motion caused by…

星系天体物理 · 物理学 2018-03-14 O. Titov , H. Krásná

Deviations from isotropy have been a key tool to identify the sources and the primary type of cosmic rays (CRs) at low energies. We argue that anisotropies due to blind regions induced by the Galactic magnetic field, the cosmological…

天体物理学 · 物理学 2008-11-26 M. Kachelriess

The highly-accurate optical reference frame GCRF (Gaia Celestial Reference Frame) is expected to be available in several years. By the same time, a new version of radio reference frame ICRF (International Celestial Reference Frame) will be…

天体物理仪器与方法 · 物理学 2015-10-06 Zinovy Malkin

The Galactic cosmic ray (GCR) intensity has been postulated by others to vary cyclically with a peak to valley ratio of ~3:1, as the Solar System moves from the Spiral Arm to the Inter-Arm regions of the Galaxy. These intensities have been…

太阳与恒星天体物理 · 物理学 2015-06-15 T. Sloan , A. W. Wolfendale

An observer stationary with respect to comoving coordinates of the expanding universe should find the redshift distribution to be isotropic. However, a peculiar motion of the observer would introduce a dipole anisotropy in the observed…

宇宙学与河外天体物理 · 物理学 2019-07-15 Ashok K. Singal

The motion of the solar system barycenter with respect to the cosmic microwave background (CMB) induces a very large apparent dipole component into the CMB brightness map at the 3 mK level. In this Letter we discuss another kinematic effect…

天体物理学 · 物理学 2009-11-11 Scott Burles , Saul Rappaport

Accelerations of both the solar system barycenter (SSB) and stars in the Milky Way cause a systematic observational effect on the stellar proper motions, which was first studied in the early 1990s and developed by J. Kovalevsky (aberration…

星系天体物理 · 物理学 2015-06-16 Jia-Cheng Liu , Yi Xie , Zi Zhu

For the nonthermal radio emission of the Galactic Center Arc in situ electron acceleration is imperative. The observed radio spectrum can be modeled by a transport equation for the relativistic electrons which includes particle acceleration…

天体物理学 · 物理学 2009-11-10 S. Lieb , H. Lesch , G. T. Birk

The conjecture is considered that every body induces the wave field which imposes oscillations on the gravitational potential of a body. The function for oscillations is chosen to prevent the gravitational collapse of the matter at the…

综合物理 · 物理学 2007-05-23 D. L. Khokhlov
‹ 上一页 1 2 3 10 下一页 ›