'Methanol masers' presentation slideshows

Methanol Masers in the NGC6334F Star Forming Region

Methanol Masers in the NGC6334F Star Forming Region. Simon Ellingsen & Anne-Marie Brick University of Tasmania Centre for Astrophysics of Compact Objects. Overview. NGC6334, a very well studied star forming region. Methanol masers in NGC6334F - so many transitions

467 views • 29 slides

Class I methanol masers in the regions of high-mass star formation

267 views • 26 slides

Rotating Disks around O-type Young Stars in NGC7538 IRS1

332 views • 20 slides

Long Baseline Array

Long Baseline Array. CSIRO ASTRONOMY & SPACE SCIENCE. Chris Phillips | LBA Lead Scientist. 26 March 2018. The Long Baseline Array (LBA).

194 views • 19 slides

Fixing the frequency coverage hole in C-Band

Fixing the frequency coverage hole in C-Band. Jagadheep D. Pandian Cornell University. Introduction. Most telescopes in U.S. currently do not have the capability to observe between 6 and 8 GHz of C-Band. This band includes the 6030 and 6035 MHz OH lines and the 6668 GHz line of methanol.

321 views • 18 slides

Using masers to characterise possible HCHII regions and pre-UCHII region stages of star formation

Using masers to characterise possible HCHII regions and pre-UCHII region stages of star formation. Shari Breen Bolton Fellow 8th September 2010. Masers as evolutionary traces of star formation?.

396 views • 17 slides

Lientjie de Villiers PhD Supervisor: Dr. M.A. Thompson University of Hertfordshire

A SEARCH FOR MOLECULAR OUTFLOWS IN THE JCMT HARP SURVEY OF 6.7 GHZ METHANOL MASERS. Lientjie de Villiers PhD Supervisor: Dr. M.A. Thompson University of Hertfordshire. CONTENTS. Methanol masers and the 6.7 GHz methanol maser survey Molecular outflows HARP instrument on the JCMT

341 views • 16 slides

Class I methanol masers in the regions of high-mass star-formation

255 views • 13 slides

The Molecular Environments of Massive Star Forming Regions Traced by Class II Methanol Masers

The Molecular Environments of Massive Star Forming Regions Traced by Class II Methanol Masers. Nichol Cunningham. Introduction. Why? Massive stars are the building blocks of the universe. Continuously chemically enrich our galaxy. Release massive amounts of energy. Where?

247 views • 13 slides

107/108 GHz methanol masers with ALMA

192 views • 10 slides

Massive star formation: First results with ATCA at 3mm

Massive star formation: First results with ATCA at 3mm. Vincent Minier School of Physics, UNSW. Tony Wong (ATNF). Michael Burton, Cormac Purcell, Tracey Hill, Lucyna Kedziora-Chudczer , Maria Hunt, Peter Barnes (UNSW). Simon Ellingsen (UTas), Dinah Cragg (Monash), Andrej Sobolev (USU).

139 views • 7 slides