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Masers as probes of the gas dynamics close to forming high-mass stars

Masers as probes of the gas dynamics close to forming high-mass stars

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_crossref_citationtrail_10_1017_S1743921317009796

Masers as probes of the gas dynamics close to forming high-mass stars

About this item

Full title

Masers as probes of the gas dynamics close to forming high-mass stars

Publisher

Cambridge, UK: Cambridge University Press

Journal title

Proceedings of the International Astronomical Union, 2017-09, Vol.13 (S336), p.201-206

Language

English

Formats

Publication information

Publisher

Cambridge, UK: Cambridge University Press

Subjects

Subjects and topics

More information

Scope and Contents

Contents

Imaging the inner few 1000 AU around massive forming stars, at typical distances of several kpc, requires angular resolutions of better than 0″.1. Very Long Baseline Interferometry (VLBI) observations of interstellar molecular masers probe scales as small as a few AU, whereas (new-generation) centimeter and millimeter interferometers allow us to ma...

Alternative Titles

Full title

Masers as probes of the gas dynamics close to forming high-mass stars

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_crossref_citationtrail_10_1017_S1743921317009796

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_crossref_citationtrail_10_1017_S1743921317009796

Other Identifiers

ISSN

1743-9213

E-ISSN

1743-9221

DOI

10.1017/S1743921317009796

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