2020MNRAS.498L..11G

Query : 2020MNRAS.498L..11G

2020MNRAS.498L..11G - Mon. Not. R. Astron. Soc., 498, L11-L14 (2020/October-2)

Analysis of methanol maser flares in G107.298+5.63 and S255-NIRS3.

GRAY M.D., ETOKA S. and PIMPANUWAT B.

Abstract (from CDS):

A 3D maser model has been used to perform an inverse problem on the light curves from three high-amplitude maser flares, selected on the basis of contemporaneous infrared observations. Plots derived from the model recover the size of the maser cloud, and two parameters linked to saturation, from three observational properties of the light curve. Recovered sizes are consistent with independent interferometric measurements. Maser objects transition between weak and moderate saturation during a flare.

Abstract Copyright: © 2020 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society

Journal keyword(s): masers - radiation mechanisms: general - radiative transfer - techniques: high angular resolution - ISM: lines and bands - radio lines: general

Status at CDS : Examining the need for a new acronym.

Simbad objects: 2

goto Full paper

goto View the references in ADS

Number of rows : 2
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 MMB G192.600-00.048 Y*O 06 12 54.0100 +17 59 23.200           ~ 430 0
2 LDN 1204A HII 22 21 26.68 +63 51 38.2           ~ 120 0

To bookmark this query, right click on this link: simbad:objects in 2020MNRAS.498L..11G and select 'bookmark this link' or equivalent in the popup menu