about
Testing properties of the Galactic center black hole using stellar orbitsThe evolution of the Milky Way from its earliest phases: Constraints on stellar nucleosynthesisReview of Particle Physics.Rapid X-ray flaring from the direction of the supermassive black hole at the Galactic Centre.A star in a 15.2-year orbit around the supermassive black hole at the centre of the Milky Way.Supernovae. Old supernova dust factory revealed at the Galactic center.Toward an Internally Consistent Astronomical Distance ScaleGlobular cluster system and Milky Way properties revisitedThe Quintuplet clusterTwo extremely luminous WN stars in the Galactic center with circumstellar emission from dust and gasThe Eddington factor as the key to understand the winds of the most massive stars. Evidence for a {Gamma}-dependence of Wolf-Rayet type mass lossStellar encounters with the solar systemThe nuclear star cluster of the Milky Way: proper motions and massCharacterization of open cluster remnantsDetection of amino acetonitrile in Sgr B2(N)Galactic spiral structureTwo estimates of the distance to the Galactic CentreComposition of the galactic center star clusterIncreased complexity in interstellar chemistry: detection and chemical modeling of ethyl formate and n-propyl cyanide in Sagittarius B2(N)Star-forming complexes and the spiral structure of our GalaxyThe Quintuplet clusterDistances of the bulge globular clusters Terzan 5, Liller 1, UKS 1, and Terzan 4 based on HST NICMOS photometryIntermediate to low-mass stellar content of Westerlund 1The Bar and Spiral Structure Legacy (BeSSeL) survey: Mapping the Milky Way with VLBI astrometryThe Quintuplet clusterLuminous blue variables: An imaging perspective on their binarity and near environmentThe spiral structure of our Milky Way GalaxyX-ray hiccups from Sagittarius A* observed by XMM-NewtonBD+43° 3654 – a blue straggler?Neutrino signal from pair-instability supernovaeThe thermal state of molecular clouds in the Galactic center: evidence for non-photon-driven heatingThe 2013 outburst of a transient very faint X-ray binary, 23 arcsec from Sgr A*Constraining MOND using the vertical motion of stars in the solar neighbourhoodGeneral relativistic magnetohydrodynamic simulations of accretion on to Sgr A*: how important are radiative losses?The metallicity distribution of bulge clump giants in Baade’s windowThe asymmetric drift, the local standard of rest, and implications from RAVE dataParticle Propagation in the Galactic Center and Spatial Distribution of Non-Thermal X-RaysAn extraordinary cluster of massive stars near the centre of the Milky WayTheGaia-ESO Survey: the Galactic thick to thin disc transition
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P2860
description
article
@en
im September 1993 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 1993
@uk
ലേഖനം
@ml
name
The Distance to the Center of the Galaxy
@en
The Distance to the Center of the Galaxy
@nl
type
label
The Distance to the Center of the Galaxy
@en
The Distance to the Center of the Galaxy
@nl
prefLabel
The Distance to the Center of the Galaxy
@en
The Distance to the Center of the Galaxy
@nl
P1476
The Distance to the Center of the Galaxy
@en
P2093
Mark J. Reid
P304
P356
10.1146/ANNUREV.AA.31.090193.002021
P407
P577
1993-09-01T00:00:00Z