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WR 140 in the Infrared

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arxiv 1101.1046 v1 pith:ZQNQBVIC submitted 2011-01-05 astro-ph.SR

Peredur Williams This is my paper · ORCID
classification astro-ph.SR
keywords infraredobservationsperiastronwr140campaignchangingdescribeddevelopment
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Observations in the infrared have played a significant role in the development of our understanding of WR140. Two sets of observations are described here: the changing profile of the 1.083-{\mu}m He I line observed for the 2009 campaign to study evolution of the wind-collision region near periastron passage, and multiwavelength photometry and imaging of the dust made by WR140 in previous periastron passages.

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  1. Dynamic Imprints of Colliding-wind Dust Formation from WR140

    astro-ph.GA 2025-02 conditional novelty 6.0 of 10

    A second JWST epoch of WR 140 shows its dust shells expanding at nearly constant speeds near the stellar wind speed, with clumpy substructures persisting for over a year.

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