Results 1 to 10 of about 29,135 (265)

Proper motions of the satellites of M31 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2019
Abstract We predict the range of proper motions of 19 satellite galaxies of M31 that would rotationally stabilize the M31 plane of satellites consisting of 15–20 members as identified by Ibata et al. Our prediction is based purely on the current positions and line-of-sight velocities of these satellites and the assumption that the plane ...
Jakub Scholtz
exaly   +4 more sources

Proper Motions of Jets on the Kiloparsec Scale: New Results with HST

open access: yesGalaxies, 2017
The Hubble Space Telescope recently celebrated 25 years of operation. Some of the first images of extragalactic optical jets were taken by HST in the mid-1990s; with time baselines on the order of 20 years and state-of-the-art astrometry techniques, we ...
Eileen T. Meyer   +9 more
doaj   +3 more sources

Independent analysis of μδ data of ILS and INDLS catalogs to obtain the spin of the bright Gaia DR2 reference frame [PDF]

open access: yesSerbian Astronomical Journal, 2021
The Gaia DR2 reference frame should be without relative rotation to the quasars (QSOs) and consistent with the International Celestial Reference System (ICRS).
Damljanović G.   +2 more
doaj   +1 more source

Improvement of Hipparcos proper motions in declination [PDF]

open access: yesSerbian Astronomical Journal, 2006
More than a decade elapsed after the HIPPARCOS ESA mission (ESA 1997) observations have been collected. This first astronomical satellite mission was less than 4 years long so that 1991.25 is the epoch of the HIPPARCOS Catalogue. Many other projects have
Damljanović Goran M.   +2 more
doaj   +1 more source

UrHip PROPER MOTION CATALOG [PDF]

open access: yesThe Astronomical Journal, 2015
11 pages, 5 figures, accepted for publication in ...
J. Frouard   +4 more
openaire   +2 more sources

THE PROPER MOTION OF PALOMAR 5 [PDF]

open access: yesThe Astrophysical Journal, 2015
Palomar 5 (Pal 5) is a faint halo globular cluster associated with narrow tidal tails. It is a useful system to understand the process of tidal dissolution, as well as to constrain the potential of the Milky Way. A well-determined orbit for Pal 5 would enable detailed study of these open questions.
Fritz, Tobias K., Kallivayalil, Nitya
openaire   +2 more sources

Photographic zenith tubes observations to improve HIPPARCOS proper motion in declination of some stars [PDF]

open access: yesSerbian Astronomical Journal, 2005
A procedure of calculation and results of an attempt to improve proper motions in declination for some HIPPARCOS stars are presented. A long series of optical observations of these stars observed with Photographic Zenith Tubes (PZT) are used.
Damljanović Goran M.
doaj   +1 more source

Position and Proper Motion of Sagittarius A* in the ICRF3 Frame from VLBI Absolute Astrometry

open access: yesThe Astronomical Journal, 2023
Sagittarius A* (Sgr A*) is a strong, compact radio source believed to be powered by a supermassive black hole at the galactic center. Extinction by dust and gas in the galactic plane prevents observing it optically, but its position and proper motion ...
David Gordon   +2 more
doaj   +1 more source

Absolute proper motions for the calibration of the Hipparcos proper motion system [PDF]

open access: yesAstronomy and Astrophysics Supplement Series, 1997
Absolute proper motions of 48 Hipparcos stars in nine elds distributed over the northern hemisphere are presented. The proper motions have been recently used as part of the Bonn program for the extragalactic link of the Hipparcos proper motion system. We describe methods which have led to the absolute proper motions of the major part of the Bonn elds ...
M. Geffert   +3 more
openaire   +1 more source

Proper Motion of Solar Filaments [PDF]

open access: yesAstronomy & Astrophysics, 1999
Precise measurements of heliographic position of solar filaments were used for describing the proper motion of solar filaments on the time-scale of one day. Only the velocity values more accurate than 100 m s−1 were used for the study. The filaments have a tendency to make a shaking or waving of the external structure and also to make a general ...
P. Ambrož, A. Schroll
openaire   +2 more sources

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