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Revisiting the Evidence for an Intermediate-mass Black Hole in the Center of NGC 6624 with Simulations
DOI: 10.1088/1674-4527/ac9274 Bibcode: 2022RAA....22k5007W

Wang, Li-Chun; Xie, Yi

The acceleration of LMXB 4U 1820-30 derived from its orbital-period derivative ${\dot{P}}_{{\rm{b}}}$ was supposed to be the evidence for an Intermediate-mass black hole (IMBH) in the Galactic globular cluster (GC) NGC 6624. However, we find that the anomalous ${\dot{P}}_{{\rm{b}}}$ is mainly due to the gravitational wave emission, rather than the…

2022 Research in Astronomy and Astrophysics
eHST 3
Evaluating Helium Variations By Modeling Red Giant Branch Bump of Large Magellanic Cluster NGC 1978
DOI: 10.1088/1674-4527/ac46a3 Bibcode: 2022RAA....22c5008J

Li, Cheng-Yuan; Ji, Xin; Deng, Li-Cai

Many evidences show that the Multiple Population (MP) features exist not only in old clusters but also in intermediate-age clusters in the Megallanic Clouds (MCs), which are characterized by star-to-star abundance scatter of several elements, including helium (He). The red giant branch bump (RGBB)'s photometric properties are proved to be related …

2022 Research in Astronomy and Astrophysics
eHST 2