Measurement of the Photosphere Oblateness of γ Cassiopeiae via Stellar Intensity Interferometry with the VERITAS Observatory

We use the stellar intensity interferometry system implemented with the Very Energetic Radiation Imaging Telescope Array System at Fred Lawrence Whipple Observatory as a light collector to obtain measurements of the rapid rotator star γ Cassiopeiae, at a wavelength of 416 nm. Using data from baselin...

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Главные авторы:	A. Archer, J. P. Aufdenberg, P. Bangale, J. T. Bartkoske, W. Benbow, J. H. Buckley, Y. Chen, N. B. Y. Chin, J. L. Christiansen, A. J. Chromey, A. Duerr, M. Escobar Godoy, S. Feldman, Q. Feng, S. Filbert, L. Fortson, A. Furniss, W. Hanlon, O. Hervet, C. E. Hinrichs, J. Holder, Z. Hughes, T. B. Humensky, W. Jin, M. N. Johnson, M. Kertzman, M. Kherlakian, D. Kieda, N. Korzoun, T. LeBohec, M. A. Lisa, M. Lundy, G. Maier, N. Matthews, P. Moriarty, R. Mukherjee, W. Ning, R. A. Ong, A. Pandey, M. Pohl, E. Pueschel, J. Quinn, P. L. Rabinowitz, K. Ragan, P. T. Reynolds, D. Ribeiro, E. Roache, J. G. Rose, I. Sadeh, L. Saha, M. Santander, J. Scott, G. H. Sembroski, R. Shang, D. Tak, J. V. Tucci, J. Valverde, V. V. Vassiliev, D. A. Williams, S. L. Wong, (The VERITAS Collaboration)
Формат:	Artigo
Язык:	Inglês
Опубликовано:	IOP Publishing 2025-01-01
Серии:	The Astrophysical Journal
Предметы:	Astronomy data modeling High angular resolution Long baseline interferometry Nonclassical interferometry Stellar radii Stellar rotation
Online-ссылка:	https://doi.org/10.3847/1538-4357/ae0744
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