M. Claussen

collaborators

2 papers

astro-ph.SR2025

First VLBI Imaging of SiO $v = 0$ , $J = 1 \to 0$ Masers in VY Canis Majoris

Hiroko Shinnaga, Miyako Oyadomari, Hiroshi Imai +8

We achieved the first VLBI detections of the ground vibrational state ( $v = 0$ ) $^{28}$ SiO (hereafter, SiO) and $^{29}$ SiO masers of the $J = 1 \to 0$ 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. PihlstrÃ¶m +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…

First VLBI Imaging of SiO v=0, J=1→0 Masers in VY Canis Majoris

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

First VLBI Imaging of SiO $v = 0$ , $J = 1 \to 0$ Masers in VY Canis Majoris