activity
19972025
most citedPolarization Observations of 1720 MHz OH Masers toward the Three Supernova Remnants W28, W44, and IC443

230 citations · 2.2k across the 58 of their papers we have counts for

collaborators

58 papers

astro-ph.SR2025

First VLBI Imaging of SiO , Masers in VY Canis Majoris

Hiroko Shinnaga, Miyako Oyadomari, Hiroshi Imai +8

We achieved the first VLBI detections of the ground vibrational state () SiO (hereafter, SiO) and SiO masers of the rotational transitions, to…

astro-ph.GA2024

Distance estimate method for Asymptotic Giant Branch stars using Infrared Spectral Energy Distributions

Rajorshi Bhattacharya, Brandon M. Medina, Ylva M. Pihlström +8

We present a method to estimate distances to Asymptotic Giant Branch (AGB) stars in the Galaxy, using spectral energy distributions (SEDs) in the near- and mid-infrared. By assumin…

astro-ph.HE2023

Front-row seat of the recent R Aqr periastron passage: X-ray multi-epoch spectral and spatial analysis

A. Sacchi, M. Karovska, J. Raymond +7

We report on the X-ray spectral and spatial evolution of the Symbiotic star R Aqr. Through a multi-epoch observational campaign performed with Chandra between 2017 and 2022, we stu…

astro-ph.GA2019★ 17 cited

The Bulge Asymmetries and Dynamical Evolution (BAaDE) SiO Maser Survey at 86 GHz with ALMA

Michael C. Stroh, Ylva M. Pihlström, Loránt O. Sjouwerman +4

We report on the first 1,432 sources observed using the Atacama Large Millimeter/submillimeter Array (ALMA), from the Bulge Asymmetries and Dynamical Evolution (BAaDE) survey, whic…

astro-ph.GA2019

From BRAVA to BAaDE: A New Kinematic Survey of the Bulge AGB

R. Michael Rich, Adam Trapp, Mark R. Morris +4

We consider interesting results on the kinematics of the bulge, beginning with Mould's (1983) measurement of the velocity dispersion of the late M giants in the bulge, and carrying…

astro-ph.SR2019

Astro2020: Molecular Masers as Probes of the Dynamic Atmospheres of Dying Stars

Lynn D. Matthews, Mark J Claussen, Graham M. Harper

More than half of the dust and heavy element enrichment in galaxies originates from the winds and outflows of evolved, low-to-intermediate mass stars on the asymptotic giant branch…