TY - JOUR

T1 - Interferometric study of the class I methanol masers at 104.3 GHz

AU - Voronkov, M. A.

AU - Breen, S. L.

AU - Ellingsen, S. P.

AU - Sobolev, A. M.

AU - Ladeyschikov, D. A.

PY - 2022/12/1

Y1 - 2022/12/1

N2 - The Australia Telescope Compact Array (ATCA) has been used for an interferometric follow up observation at 104.3 GHz of the targets where either this or the 9.9-GHz maser was previously detected. We confirm the significant difference (by more than 1.5 orders of magnitude) from source to source of the flux density ratio for these two maser transitions. Based on the morphology and location of continuum sources, the most likely explanation of this discrepancy is the difference in the flux density of the seed radiation at the two frequencies. We also report absolute positions (with arcsec accuracy) for all detected 104.3 GHz masers.

AB - The Australia Telescope Compact Array (ATCA) has been used for an interferometric follow up observation at 104.3 GHz of the targets where either this or the 9.9-GHz maser was previously detected. We confirm the significant difference (by more than 1.5 orders of magnitude) from source to source of the flux density ratio for these two maser transitions. Based on the morphology and location of continuum sources, the most likely explanation of this discrepancy is the difference in the flux density of the seed radiation at the two frequencies. We also report absolute positions (with arcsec accuracy) for all detected 104.3 GHz masers.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=85185820792

U2 - 10.1017/S1743921323001953

DO - 10.1017/S1743921323001953

M3 - Conference article

VL - 18

SP - 252

EP - 254

JO - Proceedings of the International Astronomical Union

JF - Proceedings of the International Astronomical Union

SN - 1743-9213

IS - S380

ER -