Cracking the Relation between Mass and 1P-star Fraction of Globular Clusters. II. The Masses in 1P and 2P Stars as a Second Tool by Geneviève Parmentier

“…Galactic globular clusters contain two main groups of stars, the pristine or 1P stars, and the polluted or 2P stars. …”
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Testing Cluster Membership of Planetary Nebulae with High-precision Proper Motions. I. HST Observations of JaFu 1 Near the Globular Cluster Palomar 6 by Howard E. Bond, Andrea Bellini, Kailash C. Sahu

“…In an earlier study, we used PMs to confirm that three PNe, which had already passed the other tests, are highly likely to be members of Galactic globular clusters (GCs). For a fourth object, the PN JaFu 1, which lies in the Galactic bulge near the GC Palomar 6 on the sky and has a similar RV, the available PM measurement gave equivocal results. …”
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High inclination X-ray and cataclysmic binaries by Naylor, T, Timothy Naylor

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Multiple Populations in Star Clusters by Antonino P. Milone, Anna F. Marino

Subjects: “…globular clusters…”
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Modeling and Subtracting Diffuse Cluster Light in JWST Images: A Relation between the Spatial Distribution of Globular Clusters, Dwarf Galaxies, and Intracluster Light in the Lensing Cluster SMACS 0723 by Nicholas S. Martis, Ghassan T. E. Sarrouh, Chris J. Willott, Roberto Abraham, Yoshihisa Asada, Maruša Bradač, Gabriel B. Brammer, Guillaume Desprez, Anishya Harshan, Adam Muzzin, Gaël Noirot, Gregor Rihtaršič, Marcin Sawicki, Victoria Strait

“…We apply our method to Webb’s First Deep Field the SMACS 0723 Early Release Observations and use the ICL-subtracted images to select a sample of globular clusters (GCs) and dwarf galaxies within the cluster. …”
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Erratum: “Zwicky Transient Facility and Globular Clusters: The Period–Luminosity and Period–Wesenheit Relations for Anomalous Cepheids Supplemented with Large Magellanic Cloud Sample” (2022, AJ, 164, 191) by Chow-Choong Ngeow, Anupam Bhardwaj, Matthew J. Graham, Steven L. Groom, Frank J. Masci, Reed Riddle

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JWST Identification of Extremely Low C/N Galaxies with [N/O] ≳ 0.5 at z ∼ 6–10 Evidencing the Early CNO-cycle Enrichment and a Connection with Globular Cluster Formation by Yuki Isobe, Masami Ouchi, Nozomu Tominaga, Kuria Watanabe, Kimihiko Nakajima, Hiroya Umeda, Hidenobu Yajima, Yuichi Harikane, Hajime Fukushima, Yi Xu, Yoshiaki Ono, Yechi Zhang

“…On the C/N versus O/H plane, these three galaxies do not coincide with Galactic H ii regions, normal star-forming galaxies, and nitrogen-loud quasars with asymptotic giant branch stars, but with globular-cluster (GC) stars, indicating a connection with GC formation. …”
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BV CCD Photometry of M71: Distance and Age by Hong-Suh Yim, Mun-Suk Chun, Yong-Ik Byun, Young-Jong Sohn

Subjects: “…globular cluster…”
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Calibrating X-Ray Binary Luminosity Functions via Optical Reconnaissance. II. The High-mass XLF and Globular Cluster Population of X-Ray Binaries in the Low Star-forming Spiral M81 by Qiana Hunt, Elena Gallo, Rupali Chandar, Angus Mok, Andrea Prestwich

“…We find that globular clusters that host X-ray binaries are on average more massive and more compact than globular clusters that do not. …”
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JWST Imaging of the Closest Globular Clusters. II. Discovery of Brown Dwarfs in NGC 6397 and Measurement of Age from the Brown Dwarf Cooling Sequence, Using SANDee—A New Grid of Model Isochrones across the Hydrogen-burning Limit by Roman Gerasimov, Luigi R. Bedin, Adam J. Burgasser, Daniel Apai, Domenico Nardiello, Efrain Alvarado III, Jay Anderson

“…Globular clusters contain vast repositories of metal-poor stars that represent some of the oldest stellar generations in the Universe. …”
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The effects of binary evolution on the dynamics of core collapse and neutron-star kicks by Podsiadlowski, P, Langer, N, Poelarends, A, Rappaport, S, Heger, A, Pfahl, E

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8.282J / 12.402J Introduction to Astronomy, Spring 2003 by Rappaport, S. A., 1942-, Elliot, James, 1943-

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Age and Temperature of Globular-Open Star Clusters Case Study : M3 M35 and M67 by Chewa Thassana, Wiraporn Maithong

“…In this work, the age and the temperature of the globular cluster M3 and the open clusters M37 and M67 were observed by CCD Photometer via a 0.5-meter Rithchey-Chertien Reflecting Telescope at Regional Observatory for the Public Nakhon Ratchasima, Thailand ; images were obtained of the cluster stars in B and V photometric filter. …”
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Dynamical Masses of Young Star Clusters in NGC 4038/4039 by Mengel, S, Lehnert, MD, Thatte, N, Genzel, R

“…This mass loss would make the star clusters obtain masses which are comparable to the typical mass of a globular cluster.…”

The Extended Baryonic Halo of NGC 3923 by Bryan W. Miller, Tomás Ahumada, Thomas H. Puzia, Graeme N. Candlish, Stacy S. McGaugh, J. Christopher Mihos, Robyn E. Sanderson, Mischa Schirmer, Rory Smith, Matthew A. Taylor

“…Galaxy halos and their globular cluster systems build up over time by the accretion of small satellites. …”
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The Dependence of Iron-rich Metal-poor Star Occurrence on Galactic Environment Supports an Origin in Thermonuclear Supernova Nucleosynthesis by Zachary Reeves, Kevin C. Schlaufman, Henrique Reggiani

“…These occurrences support the inference that IRMP stars formed in environments dominated by thermonuclear supernova nucleosynthesis and that the time lag between the formation of the first and second stellar generations in globular clusters was longer than the thermonuclear supernova delay time.…”
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Multimessenger Probes for New Physics in Light of A. Sakharov’s Legacy in Cosmoparticle Physics by Maxim Khlopov

“…Positive evidence for such exotic phenomena as nuclear interacting dark atoms, primordial black holes or antimatter globular cluster in our galaxy would provide the selection of viable BSM models determination of their parameters.…”
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Intermediate Mass Black Holes: Their Motion and Associated Energetics by C. Sivaram, Kenath Arun

“…The active galaxy M82 and the globular cluster G1 in M31, for example, are known to host such objects. …”
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DISCOVERY OF A HIGHLY VARIABLE DIPPING ULTRALUMINOUS X-RAY SOURCE IN M94 by Lin, Dacheng, Irwin, Jimmy A., Webb, Natalie A., Barret, Didier, Remillard, Ronald A

“…Thus, our source is a candidate stellar-mass BHB with a supergiant companion or with a dwarf companion residing in a globular cluster. Our study supports that some low-luminosity ULXs are supercritically accreting stellar-mass BHBs.…”
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Kicking Time Back in Black Hole Mergers: Ancestral Masses, Spins, Birth Recoils, and Hierarchical-formation Viability of GW190521 by Carlos Araújo-Álvarez, Henry W. Y. Wong, Anna Liu, Juan Calderón Bustillo

“…If GW190521 was eccentric, we obtain p _2 _g ≃ 0.1 for any host other than an active galactic nucleus, and zero for a globular cluster. If GW190521 was quasi circular, a nuclear star cluster origin is possible with p _2 _g ∈ (∼0.4, ∼0.8).…”
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