Testing ultralow amplitude Cepheid candidates in the Galactic disk by TESS and Gaia
Ultralow amplitude (ULA) and strange mode Cepheids are thought to be pulsating variable
stars that are near to or are at the edges of the classical instability strip. Until now, a few …
stars that are near to or are at the edges of the classical instability strip. Until now, a few …
Testing ultralow amplitude Cepheid candidates in the Galactic disk by TESS and Gaia
D Tarczay-Nehéz, L Molnár, A Bódi… - Astronomy and …, 2023 - ui.adsabs.harvard.edu
Ultralow amplitude (ULA) and strange mode Cepheids are thought to be pulsating variable
stars that are near to or are at the edges of the classical instability strip. Until now, a few …
stars that are near to or are at the edges of the classical instability strip. Until now, a few …
Testing Ultra-low Amplitude Cepheid Candidates in the Galactic Disk by TESS and Gaia
D Tarczay-Nehéz, L Molnár, A Bódi… - arXiv preprint arXiv …, 2023 - arxiv.org
Ultra-low amplitude (ULA) and strange mode Cepheids are thought to be pulsating variable
stars that are near to or are at the edges of the classical instability strip. Until now, a few …
stars that are near to or are at the edges of the classical instability strip. Until now, a few …