About: IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way

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About: IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way Goto Sponge NotDistinct Permalink

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scientific article published in the Astrophysical Journal

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rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) наукова стаття, опублікована у квітні 2005 (uk) im April 2005 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astrophysical Journal (fr) scientific article published in the Astrophysical Journal (en)
publication date	wds:Q59939312-87C397A1-400E-48BC-B4A6-69A0876609D5
publication date	2005-04-28 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q59939312-5B603A83-7BCA-4DED-9296-D8F8CE1952AB
language of work or name	English
cites work	wds:Q59939312-084C630C-6A31-4EDB-A5FE-0F38C5EAE279 wds:Q59939312-15C19B36-B96B-4571-8155-240047BE972F wds:Q59939312-16251ABB-F956-45E5-B0F0-9D37C3ECEE80 wds:Q59939312-1BC439D5-267B-4053-96AC-239FB149EA4E wds:Q59939312-234649BD-D93D-421E-8374-B52A6606E9F2 wds:Q59939312-34A39CDD-E2C6-44A3-BED4-2550D510D92F wds:Q59939312-3AA53590-5ED9-4684-A9C2-CDA89D5F9D6C wds:Q59939312-44BBA02A-FE88-4867-935D-839FC7CC2E9A wds:Q59939312-4712BA75-2E16-474B-BADD-114F32E5130B wds:Q59939312-4CDBC0D4-AF92-4AD1-8EF5-DA35836962BD wds:Q59939312-5403D2FE-0F15-4B05-80C8-2EA0CC7461DB wds:Q59939312-556E991F-0DE6-4883-9B6A-BD7F98E795D5 wds:Q59939312-6111D93D-FEEE-4F4C-ACF8-203A94632630 wds:Q59939312-65659507-A2C1-4BD6-9BB3-62E7E966FE9B wds:Q59939312-70BCF36F-7006-4E2D-89B1-3B52D187666D wds:Q59939312-825624D1-8BF2-4F43-AA57-4347B78D2A73 wds:Q59939312-82933832-C730-4215-9DAE-BC8AD98966E7 wds:Q59939312-86E5D399-4602-408C-B27C-471F0A7132F8 wds:Q59939312-89C6D399-DC5D-4839-9C70-F98E88DB8D42 wds:Q59939312-9BB089A7-2E52-4CC3-99C4-973B5BB55067 wds:Q59939312-A246EA2F-ED37-4134-84E3-9413BDC55861 wds:Q59939312-B29612F5-6F1A-426D-86C9-F0D221FC635F wds:Q59939312-BA5B9494-B23A-475D-AD4C-73CF8F4A5D61 wds:Q59939312-C4B6579A-1D79-4EA4-8411-426B45EF4605 wds:Q59939312-D590324C-D43D-4093-8FB3-EAA7E01C621B wds:Q59939312-E7E9EA50-B937-4430-9A5B-B3CBA9762913 wds:Q59939312-EB4A1334-4F9E-4B95-B9C4-EA5E027B389A wds:Q59939312-FB0A2F3D-B3AE-4BE0-AF11-C230C5F7654C wds:Q59939312-FFA93D05-0F1F-4AF2-963C-3C580297DE03 wds:Q59939312-FFB90E81-23A6-454F-9696-689BB69AA56D
cites work	The Distance to the Center of the Galaxy Stellar dynamics in the Galactic Centre: proper motions and anisotropy The accelerations of stars orbiting the Milky Way's central black hole Stellar Orbits around the Galactic Center Black Hole High Proper-Motion Stars in the Vicinity of Sagittarius A: Evidence for a Supermassive Black Hole at the Center of Our Galaxy The First Measurement of Spectral Lines in a Short-Period Star Bound to the Galaxy’s Central Black Hole: A Paradox of Youth The first diffraction-limited images from the W.M. Keck Telescope Analysis of isoplanatic high resolution stellar fields by the StarFinder code Massive star formation near the Galactic Center and the fate of the stellar remnants The case against a massive black hole at the Galactic Centre High‐Precision Stellar Radial Velocities in the Galactic Center The Nuclear Cluster of the Milky Way: Star Formation and Velocity Dispersion in the Central 0.5 Parsec Methods for determining the masses of spherical systems. I. Test particles around a point mass The stellar cusp around the supermassive black hole in the Galactic Center The Proper Motion of Sagittarius A. II. The Mass of Sagittarius A* Chandra X-ray spectroscopic imaging of Sagittarius A* and the central parsec of the galaxy The mass of the open star cluster M35 as derived from proper motions Stellar Dynamics in the Central Arcsecond of Our Galaxy The Galactic Center He I stars: remains of a dissolved young cluster? Dynamical friction on star clusters near the Galactic Center Dynamical friction on Galactic Center star clusters with an intermediate-mass black hole Stellar disk in the Galactic center: a remnant of a dense accretion disk The origin of IRS 16: dynamically driven in-spiral of a dense star cluster to the Galactic Center The fate of star clusters near the Galactic Center. I. Analytic considerations A deep Chandra catalog of X-ray point sources toward the Galactic Center The nature of the Galactic Center source IRS 13 revealed by high spatial resolution in the infrared The need for a second black hole at the Galactic Center Young stars at the center of the Milky way The lives and deaths of star clusters near the Galactic Center An extended star formation history for the Galactic Center from Hubble Space Telescope NICMOS observations
author name string	wds:Q59939312-3227EEAE-275B-4D95-97AD-4B13E1B22D7B wds:Q59939312-35190C81-2F4D-4809-B0AD-E6746DE2B909 wds:Q59939312-566416A0-8E00-4B2C-879A-A4528DA38B82 wds:Q59939312-67A90306-188D-4BA6-BFE9-CB89C4B0CD41
author name string	M. Morris E. E. Becklin J. R. Lu S. D. Hornstein
rdfs:label	IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (en) IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (nl)
skos:prefLabel	IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (en) IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (nl)
name	IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (en) IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (nl)
author	wds:Q59939312-80B9B40C-F844-458D-BC60-752AB242108D
author	Andrea M. Ghez
title	wds:Q59939312-CBDEDFDF-9DF7-4E7D-B88D-214D0818C2B9
title	IRS 16 SW: A New Comoving Group of Young Stars in the Central Parsec of the Milky Way (en)
page(s)	wds:Q59939312-4F5C0E00-0841-4A6E-8020-4FF3E708E378
page(s)	51–54
instance of	wds:Q59939312-9AD8F70D-61C8-4CF1-92BD-D7D0E401C4EE
instance of	scholarly article
published in	wds:Q59939312-3A5F9D43-AB11-42CC-8352-BEA1F1B6B74F
full work available at URL	wds:Q59939312-E8F1013B-194E-4A1C-B73D-0FE285C3E1BD
published in	The Astrophysical Journal
full work available at URL	https://iopscience.iop.org/article/10.1086/430879/pdf
issue	wds:Q59939312-AAD9F223-1F89-4F72-BCD5-903F570E266E
volume	wds:Q59939312-DDA96F0A-FE39-43D8-AF82-DC9D2182765E
issue	1

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