2022MNRAS.516L..96M

Query : 2022MNRAS.516L..96M

2022MNRAS.516L..96M - Mon. Not. R. Astron. Soc., 516, L96-L100 (2022/October-2)

Two periods instead of one in a single 6.7 GHz methanol maser feature in G9.62+0.20E.

MacLEOD G.C., YONEKURA Y., TANABE Y., BAAN W.A., BROGAN C.L., BURNS R.A., CHIBUEZE J.O., HOUDE M., HUNTER T.R., KURTZ S.E., RAJABI F., SMITS D.P., STECKLUM B. and SUGIYAMA K.

Abstract (from CDS):

The source G9.62+0.20E surprises yet again! Analysis of the associated methanol maser feature at vlsr = +8.8 km s–1 revealed a second period of P = 52.1 ± 0.3 d, along with the previously reported period P = 243 d for this source. Various explanations, harmonic flaring, Dicke's superradiance, a secondary pulsation, or two different periodically varying radio sources in the field of view with associated methanol masers are presented. The latter two hypotheses appear more plausible but it is not clear which, if any, best describe these observations.

Abstract Copyright: © 2022 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): masers - stars: formation - stars: protostars - ISM: individual objects: G9.62+0.20E - ISM: molecules - radio lines: ISM

Simbad objects: 4

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Number of rows : 4
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 OH 009.621+00.196 Mas 18 06 14.6600 -20 31 31.700           ~ 56 0
2 [GRM93] G09.61+0.20 E HII 18 06 14.7 -20 31 32           ~ 51 0
3 OH 009.619+00.193 Mas 18 06 14.92 -20 31 44.3           ~ 10 0
4 V* RR Lyr RR* 19 25 27.9129605304 +42 47 03.693258204   7.36   7.6   kA3hF0 951 0

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