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Proper motion
The Dunhuang Chinese Sky: a Comprehensive Study of the Oldest Known Star Atlas
Constraining the Masses of Microlensing Black Holes and the Mass Gap with Gaia DR2 Łukasz Wyrzykowski1 and Ilya Mandel2,3,4
New Wide Common Proper Motion Binaries
Lecture 8: Stellar Motions Reading: Box 19-1
Arxiv:1703.10167V1
Near IR Astrometry of Magnetars Shriharsh P
The Proper Motion of M31 Roeland Van Der Marel (Stsci)
On Gp Kuiper's Work on the Stars of Large Proper Motion
Proper Motion of a Star
Arxiv:2101.05282V3 [Astro-Ph.SR] 2 Feb 2021 at Angular Separations Greater Than About One Arcsecond, Wide Et Al
Arxiv:0902.1781V2 [Astro-Ph.GA] 30 Mar 2009 Martinez-Delgado .Munn A
New Determinations of the Proper Motions of 44 Pulsars PA
The Acceleration of the Solar System Barycenter Determined By
Wide Binary Companions to Tycho-Gaia Stars
THE FORMATION of STELLAR BLACK HOLES 1. Introduction
An Astrometric and Spectroscopic Study of the Galactic Cluster Ngc 1039
Willem Luyten’S Interest in Astronomy Dates from the 1910 Appearance of Halley’S Comet Over His Home in Semarang
International Legislation in the Field of Astronomical Nomenclature
Top View
The Proper Motion of the Galactic Center Pulsar Relative to Sagittarius A*
Proper Motion of Barnards Star
Gaia DFS PLS Prop
Measuring the Sun's Motion with Stellar Streams
The Acs Survey of Galactic Globular Clusters. Iii. the Double Subgiant Branch of Ngc 18511 A
Gaia Reference Frame Amid Quasar Variability and Proper Motion Patterns in the Data R
Proper Motion Determination of Open Clusters Based on the UCAC2 Catalogue
Study of Common Proper Motion Visual Double Stars - the CPDS Catalogue
Proper Motions and Membership Probabilities of Stars in the Region of Globular Cluster NGC 6366 ,
The 28-Xiu Constellations in East Asian Calendars and Analysis of Their Observation Dates
The Center of Expansion and Age of the Oxygen-Rich Supernova Remnant 1E 0102.2-7219
MASS DETERMINATIONS of POPULATION II BINARY STARS Kathryn E
Proper Motion of Pulsar B1800-21
22. Time Domain Surveys
The Family of Stars What Is a Star? How Far Away Are They? How Hot Are They? How Large Are They? How Much Do They Weigh?
Arxiv:2012.01586V2 [Astro-Ph.GA] 14 Dec 2020 the Local Group, Most Are Satellites of the Milky Way Or M31
110823 Pune Precision Astrometry
Galactic Rotation and Solar Motion
The Dunhuang Chinese Sky: a Comprehensive Study of the Oldest Known Star Atlas
Binary Pulsar Distances and Velocities from Gaia Data Release 2
Beta Hydri G2 Iv : a Revised Age for the Closest Subgiant
How to Understand Stars Chapter 17 Location in Space How Parallax
5 the Motion of Stars
A Kinematic Study of Central Compact Objects and Their Host Supernova Remnants Martin G
Arxiv:2008.06438V1 [Astro-Ph.IM] 14 Aug 2020 1 INTRODUCTION
Arxiv:1502.05069V1 [Astro-Ph.SR] 17 Feb 2015 02,21;Zege L 04.Teesashv Radial Have S 2009, Stars Km These Al
One and the Same Apparent Magnitude, Mi. the Arithmetic Mean Value of the Reduced T Components Is Then Compared with That of the Radial Velocities
Accurate Spectral Classification by Objective-Prism Techniques
Gaia Early Data Release 3: Acceleration of the Solar System
The Proper Motion of the Local Group Galaxy IC 10
1 Observational Evidence for Black Holes
Acceleration of the Solar System from Gaia Astrometry? Gaia Collaboration: S
The Center of Expansion and Age of the Oxygen-Rich Supernova Remnant 1E 0102.2-7219 ABSTRACT We Present New Proper Motion Measur
A Statistical Study of Pulsar Proper Motions
Discovery of New Companions to High Proper Motion Stars from the VVV Survey ,
Proper Motion Surveys
Discovery of a Candidate Black Hole−Giant Star Binary System in the Galactic Field
The Proper Motion of the Central Compact Object RX J0822-4300 in the Supernova Remnant Puppis A
Psrs J0248+6021 and J2240+5832: Young Pulsars in the Northern Galactic Plane Discovery, Timing, and Gamma-Ray Observations
19 6 9Apj. . .158.1115S the Astrophysical Journal
Proper Motion in Lensed Radio Jets at Redshift 3: a Possible Dual Super-Massive Black Hole System in the Early Universe? C
Stars in Motion
Toward an Empirical Theory of Pulsar Emission Xi