Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-25T17:14:21.481Z Has data issue: false hasContentIssue false
  • English
  • Français

Global outburst of methanol maser in G24.33+0.14

Published online by Cambridge University Press:  16 July 2018

P. Wolak ,
M. Szymczak ,
M. Olech  and
A. Bartkiewicz
P. Wolak
Affiliation:
Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland email: [email protected]
M. Szymczak
Affiliation:
Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland email: [email protected]
M. Olech
Affiliation:
Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland email: [email protected]
A. Bartkiewicz
Affiliation:
Centre for Astronomy, Faculty of Physics, Astronomy and Informatics, Nicolaus Copernicus University, Grudziadzka 5, 87-100 Torun, Poland email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A strong outburst of 6.7 GHz methanol maser occurred in the high-mass young stellar object (HMYSO) G24.33+0.14 between November 2010 and January 2013. The target was observed with the Torun 32 m radio telescope as a part of a long-term monitoring programme. Almost all twelve spectral features from 108 to 120 km s−1 varied synchronously with time delays between the flux minima of about two weeks. This may indicate that the variability is driven by global changes in the pump rate. The flare peaks of the two features with the highest relative amplitude of 40-60 are delayed by about 2.5 months while their profiles undergo essential transformation with a velocity drift of 0.23 km s−1yr−1. This may suggest that the variability is caused by a rapid increase of the pump rate and excitation of a large portion of the HMYSO environment by an accretion event.

Keywords

masersstars: formationISM: cloudsradio lines: ISM
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 13 , Symposium S336: Astrophysical Masers: Unlocking the Mysteries of the Universe , September 2017 , pp. 319 - 320
Copyright
Copyright © International Astronomical Union 2018 

References

Bartkiewicz, A., Szymczak, M., & van Langevelde, H. J., 2016, ApJ, 587, A104Google Scholar
Caswell, J. L. & Green, J. A., 2011, MNRAS, 411, 2059CrossRefGoogle Scholar
Hu, B., Menten, K. M., Wu, Y., Bartkiewicz, A., Rygl, K., Reid, M. J., Urquhart, J. S., & Zheng, X., 2016, ApJ, 833, 18CrossRefGoogle Scholar
Moscadelli, L., Sanna, A., Goddi, C., Walmsley, M. C., Cesaroni, R., Caratti o Garatti, A., Stecklum, B., Menten, K. M., & Kraus, A., 2017, A&A, 600, L8Google Scholar