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ZENODO
Conference object . 2021
License: CC BY
Data sources: Datacite
image/svg+xml art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos Open Access logo, converted into svg, designed by PLoS. This version with transparent background. http://commons.wikimedia.org/wiki/File:Open_Access_logo_PLoS_white.svg art designer at PLoS, modified by Wikipedia users Nina, Beao, JakobVoss, and AnonMoos http://www.plos.org/
ZENODO
Conference object . 2021
License: CC BY
Data sources: Datacite
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Binarity in massive young stellar objects

descriptionPublicationkeyboard_double_arrow_right Conference object 11 Oct 2021 English Publisher:Zenodo
Authors: Shenton, Robert;

doi: 10.5281/zenodo.5562345 , 10.5281/zenodo.5562346

Binarity in massive young stellar objects

Abstract

Most massive stars (up to 100%) are thought to be in binary systems. The multiplicity of massive stars seems to be intrinsically linked to their formation and evolution, and so Massive Young Stellar Objects are key in observing this early stage of star formation. We have surveyed three samples of hundreds of MYSOs across the Galaxy from the RMS catalogue, using UKIDSS and VVV point source data, and UKIRT K-band imaging.

Keywords

massive stars, binary, star formation

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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