The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis

Bibliographic Details
Title: The Great Dimming of the Hypergiant Star RW Cephei: CHARA Array Images and Spectral Analysis
Authors: Narsireddy Anugu, Fabien Baron, Douglas R. Gies, Cyprien Lanthermann, Gail H. Schaefer, Katherine A. Shepard, Theo ten Brummelaar, John D. Monnier, Stefan Kraus, Jean-Baptiste Le Bouquin, Claire L. Davies, Jacob Ennis, Tyler Gardner, Aaron Labdon, Rachael M. Roettenbacher, Benjamin R. Setterholm, Wolfgang Vollmann, Costantino Sigismondi
Source: The Astronomical Journal, Vol 166, Iss 2, p 78 (2023)
Publisher Information: IOP Publishing, 2023.
Publication Year: 2023
Collection: LCC:Astronomy
Subject Terms: Late-type supergiant stars, Stellar mass loss, Stellar radii, Variable stars, Astronomy, QB1-991
More Details: The cool hypergiant star RW Cephei is currently in a deep photometric minimum that began several years ago. This event bears a strong similarity to the Great Dimming of the red supergiant Betelgeuse that occurred in 2019–2020. We present the first resolved images of RW Cephei that we obtained with the CHARA Array interferometer. The angular diameter and Gaia distance estimates indicate a stellar radius of 900–1760 R _⊙ , which makes RW Cephei one of the largest stars known in the Milky Way. The reconstructed, near-infrared images show a striking asymmetry in the disk illumination with a bright patch offset from the center and a darker zone to the west. The imaging results depend on assumptions made about the extended flux, and we present two cases with and without allowing extended emission. We also present a recent near-infrared spectrum of RW Cep that demonstrates that the fading is much larger at visual wavelengths compared to that at near-infrared wavelengths as expected for extinction by dust. We suggest that the star’s dimming is the result of a recent surface mass ejection event that created a dust cloud that now partially blocks the stellar photosphere.
Document Type: article
File Description: electronic resource
Language: English
ISSN: 1538-3881
Relation: https://doaj.org/toc/1538-3881
DOI: 10.3847/1538-3881/ace59d
Access URL: https://doaj.org/article/3d78bb109b98401f9c555876aca37665
Accession Number: edsdoj.3d78bb109b98401f9c555876aca37665
Database: Directory of Open Access Journals
More Details
ISSN:15383881
DOI:10.3847/1538-3881/ace59d
Published in:The Astronomical Journal
Language:English