activity
20062023
most citedSub-arcsecond (sub)millimeter imaging of the massive protocluster G358.93-0.03: Discovery of 14 new methanol maser lines associated with a hot core

61 citations · 194 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2023

Long-term multiwavelength monitoring and reverberation mapping of NGC 2617 during a changing-look event

V. L. Oknyansky, M. S. Brotherton, S. S. Tsygankov +32

We present the results of photometric and spectroscopic monitoring campaigns of the changing look AGN NGC~2617 carried out from 2016 until 2022 and covering the wavelength range fr…

astro-ph.GA2023★ 8 cited

Ammonia masers toward G358.931-0.030

T. P. McCarthy, S. L. Breen, J. F. Kaczmarek +9

We report the detection of ammonia masers in the non-metastable (6, 3), (7, 5) and (6, 5) transitions, the latter is the first unambiguous maser detection of that transition ever m…

astro-ph.GA2022★ 18 cited

A multi-transition methanol maser study of the accretion burst source G358.93-0.03-MM1

O. S. Bayandina, C. L. Brogan, R. A. Burns +8

We present the most complete to date interferometric study of the centimeter wavelength methanol masers detected in G358.93-0.03 at the burst and post-burst epochs. A unique, NIR/(…

astro-ph.GA2021★ 7 cited

Variability in extragalactic class I methanol masers: New maser components toward NGC4945 and NGC253

Tiege McCarthy, Simon Ellingsen, Shari Breen +3

We have used the Australia Telescope Compact Array (ATCA) to make new observations of the 36.2-GHz (E) methanol transition toward NGC 4945 and NGC 253. These…

astro-ph.GA2019★ 34 cited

Local RR Lyrae Stars: native and alien

R. Zinn, X. Chen, A. C. Layden +1

Measurements of [Fe/H] and radial velocity are presented for 89 RR Lyrae (RRL) candidates within 6 kpc of the Sun. After removal of two suspected non-RRL, these stars were added to…

astro-ph.GA2019★ 9 cited

36 GHz methanol lines from nearby galaxies: maser or quasi-thermal emission?

P. Humire, C. Henkel, Y. Gong +12

Methanol (CH3OH) is one of the most abundant interstellar molecules, offering a vast number of transitions to be studied, including many maser lines. While the strongest Galactic C…