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astro-ph.GA2026

Indications of electron-to-proton mass ratio variations in the Galaxy. III. 0.6mm methanol lines toward SgrB2(N) and Orion-KL

J. S. Vorotyntseva, S. A. Levshakov

In this paper, we show that methanol (CH3OH) torsional-rotational transitions, which have increased sensitivity to small variations of mu - the electron-to-proton mass ratio, are s…

astro-ph.GA2025

Indications of electron-to-proton mass ratio variations in the Galaxy. II. 3 mm methanol lines toward Sgr B2(N) and (M)

J. S. Vorotyntseva, S. A. Levshakov, C. Henkel

Differential measurements of the fundamental constant mu = m_e/m_p (the electron-to-proton mass ratio) for two sources near the Galactic Center - the Sgr B2(N) and B2(M) molecular…

astro-ph.GA2025

Indication of the electron-to-proton mass ratio variation within the Galaxy

J. S. Vorotyntseva, S. A. Levshakov

Near (~100 pc) and far (~8.7 kpc) relative to the Galactic center, the molecular clouds SgrB2(N) and Orion-KL exhibit different values of the fundamental physical constant mu=m_e/m…

astro-ph.GA2024

Hyperfine structure of the methanol molecule as traced by Class I methanol masers

I. I. Agafonova, O. S. Bayandina, Y. Gong +9

We present results on simultaneous observations of Class~I methanol masers at 25, 36, and 44 GHz towards 22 Galactic targets carried out with the Effelsberg 100-m telescope. The st…

astro-ph.GA2024

Torsion-rotational transitions in methanol as a probe of fundamental physical constants -- electron and proton masses

J. S. Vorotyntseva, S. A. Levshakov

We report on the using of torsion-rotational transitions in the CH3OH and (13)CH3OH molecules to evaluate possible variations of the physical constant mu=m_e/m_p - the electron-to-…