12–23 Jul 2021
Online
Europe/Berlin timezone

The VERITAS-Stellar Intensity Interferometry (VSII) survey of Stellar Diameters

16 Jul 2021, 18:00
1h 30m
TBA

TBA

Poster GAI | Gamma Ray Indirect Discussion

Speaker

David Kieda (University of Utah)

Description

The VERITAS Imaging Air Cherenkov Telescope (IACT) array was augmented in 2019 with high-speed focal plane electronics to allow the use of VERITAS for Stellar Intensity Interferometry (SII) observations. Since January 2019, VSII recorded more than 127 hours of moonlit observations on 22 different bright stars and binary systems ($m_V$ < 3). The observations resulting in the measurement of the diameters of several stars at an effective optical wavelength of 417 nm with better than 5% resolution. This talk will describe the results of selected VSII observations, and discuss the sensitivity of these results to stellar phenomena such as limb darkening, rapid rotation, and other astrophysical effects.

Keywords

Intensity Interferometry; stellar diameters; IACT arrays; stellar envelopes; limb darkening

Subcategory Experimental Results
Collaboration VERITAS

Primary authors

Presentation materials