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

28 papers

astro-ph.GA2025★ 5 cited

The Expanding 3 kpc Arms Are Neither Expanding nor Spiral Arms but X1 Orbits Driven by the Galactic Bar

Jayender Kumar, Mark J. Reid, T. M. Dame +6

Near the center of our Milky Way is a bar-like structure and the so-called Expanding 3-kpc arms. We currently have limited knowledge of this important region, since we are about 8.…

astro-ph.GA2019★ 20 cited

Accretion disk versus jet orientation in HO megamaser galaxies

F. Kamali, C. Henkel, S. Koyama +10

An essential part of the paradigm describing active galactic nuclei is the alignment between the radio jet and the associated rotation axis of the sub-pc sized accretion disks. Bec…

astro-ph.SR2018★ 20 cited

The Evolving Radio Photospheres of Long-Period Variable Stars

L. D. Matthews, M. J. Reid, K. M. Menten +1

Observations with the Karl G. Jansky Very Large Array at 46 GHz (7 mm) have been used to measure the size and shape of the radio photospheres of four long-period variable stars: R…

astro-ph.GA2016★ 291 cited

A Parallax-based Distance Estimator for Spiral Arm Sources

M. J. Reid, T. M. Dame, K. M. Menten +1

The spiral arms of the Milky Way are being accurately located for the first time via trigonometric parallaxes of massive star forming regions with the BeSSeL Survey, using the Very…

astro-ph.SR2016★ 43 cited

The Population of Compact Radio Sources in the Orion Nebula Cluster

Jan Forbrich, Victor M. Rivilla, Karl M. Menten +6

We present a deep centimeter-wavelength catalog of the Orion Nebula Cluster (ONC), based on a 30h single-pointing observation with the Karl G. Jansky Very Large Array in its high-r…

astro-ph.SR2015★ 22 cited

New Measurements of the Radio Photosphere of Mira based on Data from the JVLA and ALMA

L. D. Matthews, M. J. Reid, K. M. Menten

We present new measurements of the millimeter wavelength continuum emission from the long period variable Mira ( Ceti) at frequencies of 46 GHz, 96 GHz, and 229 GHz (~7 mm, 3…