Photometry and spectroscopy of a deep Algol-like minimum of WW Vul in 2016

Fuente: arXiv
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Main Author: Boyd, David
Format: Preprint
Published: 2024
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author Boyd, David
author_facet Boyd, David
contents We report analysis of photometry and spectroscopy of a deep Algol-like minimum of the pre-main-sequence star WW Vul in July and August 2016. This revealed substantial reddening due to absorption by circumstellar material. After dereddening, our spectra of WW Vul were consistent with spectral type A3V throughout the event. Hα is normally in emission in WW Vul. During the minimum, Hα emission dropped by ~30% and FWHM of the Hα line reduced by ~15%.
format Preprint
id arxiv_https___arxiv_org_abs_2409_10073
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Photometry and spectroscopy of a deep Algol-like minimum of WW Vul in 2016
Boyd, David
Solar and Stellar Astrophysics
We report analysis of photometry and spectroscopy of a deep Algol-like minimum of the pre-main-sequence star WW Vul in July and August 2016. This revealed substantial reddening due to absorption by circumstellar material. After dereddening, our spectra of WW Vul were consistent with spectral type A3V throughout the event. Hα is normally in emission in WW Vul. During the minimum, Hα emission dropped by ~30% and FWHM of the Hα line reduced by ~15%.
title Photometry and spectroscopy of a deep Algol-like minimum of WW Vul in 2016
topic Solar and Stellar Astrophysics
url https://arxiv.org/abs/2409.10073