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ZENODO
Conference object . 2021
License: CC BY
Data sources: Datacite
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ZENODO
Other literature type . 2021
License: CC BY
Data sources: ZENODO
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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Dust formation in a long-period colliding wind binary WR 125

descriptionPublicationkeyboard_double_arrow_right Conference object , Other literature type 08 Dec 2021Publisher:Zenodo
Authors: Arora, Bharti; J. C. Pandey; M. De Becker; S. B. Pandey; N. K. Chakradhari; S. Sharma; B. Kumar;

doi: 10.5281/zenodo.5768178 , 10.5281/zenodo.5768177

Dust formation in a long-period colliding wind binary WR 125

Abstract

A long-term infrared and X-ray investigation of the colliding-wind binary WR 125 (WC7+O9III) has been performed. The source appeared brighter in the near and mid infrared wavebands during the years 2017–2021. The infrared excess is attributed to another episode of dust formation after similar instance reported at the beginning of the 1990s during its periastron passage. Long-term modulations have also been observed in the X-ray flux measurements. Both infrared and X-ray emission variations suggest an orbital period ~28-29 years. Multiwavelength observations of WR 125 allowed to draw relevant guidelines for future exploration of this massive binary.

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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.
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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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