On the Class II methanol maser periodic variability due to the rotating spiral shocks in the gaps of discs around young binary stars

Research output: Contribution to journal › Article › peer-review

Original language	English
Pages (from-to)	620-628
Number of pages	9
Journal	Monthly Notices of the Royal Astronomical Society
Volume	444
Issue number	1
DOIs	https://doi.org/10.1093/mnras/stu1481
Publication status	Published - 11 Oct 2014

accretion, accretion discs, masers, binaries: general, ORION NEBULA, 6.7 GHZ, VLBI OBSERVATIONS, FORMING REGIONS, STELLAR OBJECTS, MASSIVE STARS, G9.62+0.20E, EMISSION, ACCRETION, DISKS

ID: 394266