Stability of Nonradial Pulsations in the Be Star [MA93]1506-Reference-Cited by-同舟云学术

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Stability of Nonradial Pulsations in the Be Star [MA93]1506

Published:2021-11-16 Issue:11 Volume:5 Page:266
ISSN:2515-5172
Container-title:Research Notes of the AAS
language:
Short-container-title:Res. Notes AAS

Author:

Schmidtke P. C.^ORCID,Cowley A. P.,Udalski A.^ORCID

Abstract

Abstract Period analysis of the 1993–2020 MACHO and OGLE photometry for Be star [MA93]1506 reveals non-radial pulsations are present in all observing seasons, with a mean period of 1.09942 ± 0.00018 days.

Publisher

American Astronomical Society

Link

https://iopscience.iop.org/article/10.3847/2515-5172/ac391c/pdf

Reference16 articles.

1. Calibration of the MACHO Photometry Database

2. Short-period variables in the Small Magellanic Cloud cluster NGC 330

3. On the periodicities present in the optical light curves of Small Magellanic Cloud Be/X-ray binaries

4. Optical properties of Small Magellanic Cloud X-ray binaries

5. Pulsating B and Be stars in the Small Magellanic Cloud

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