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M. J. Reid

28 papers hereh-index 161.7k citations33 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author4
  • middle author15
  • last author3

Across the 22 of 28 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA14
  • astro-ph7
  • astro-ph.SR4
  • astro-ph.CO2
  • astro-ph.IM1
same name
  • M. J. Reid — 1 paper
  • M. J. Reid — 1 paper, h 3

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20012025
most citedAn Extremely Top-Heavy IMF in the Galactic Center Stellar Disks

383 citations · 2.1k across the 28 of their papers we have counts for

collaborators
Showing 2009Show all

4 papers · 1 filter

astro-ph.GA2009★ 383 cited

An Extremely Top-Heavy IMF in the Galactic Center Stellar Disks

H. Bartko, F. Martins, S. Trippe +19

We present new observations of the nuclear star cluster in the central parsec of the Galaxy with the adaptive optics assisted, integral field spectrograph SINFONI on the ESO/VLT. O…

astro-ph.GA2009★ 6 cited

The Galactic Center: A Laboratory for Fundamental Astrophysics and Galactic Nuclei

A. Ghez, M. Morris, J. Lu +24

As the closest example of a galactic nucleus, the Galactic center presents an exquisite laboratory for learning about supermassive black holes (SMBH) and their environs. Detailed s…

astro-ph.GA2009★ 4 cited

CO in OH/IR stars close to the Galactic centre

A. Winnberg, S. Deguchi, M. J. Reid +3

Aims: A pilot project has been carried out to measure circumstellar CO emission from three OH/IR stars close to the Galactic centre. The intention was to find out whether it would…

astro-ph.GA2009★ 56 cited

The distance to a star forming region in the Outer arm of the Galaxy

K. Hachisuka, A. Brunthaler, K. M. Menten +3

We performed astrometric observations with the VLBA of WB89-437, an H2O maser source in the Outer spiral arm of the Galaxy. We measure an annual parallax of 0.167 +/- 0.006 mas, co…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.