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  1. 41

    Evolution of Extremely Soft Binaries in Dense Star Clusters: On the Jupiter Mass Binary Objects by Yihan Wang, Rosalba Perna, Zhaohuan Zhu, Douglas N. C. Lin

    Published 2025-01-01
    “…Our findings reveal that for low-mass soft binaries, the semimajor axis distribution asymptotes to a universal power law between  ∝ a ^−8/3 and  ∝ a ^−5/3 over the derived ionization timescale. …”
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    Development Binary Search Algorithm by Baghdad Science Journal

    Published 2011-06-01
    “…It consists of three locations (1-Top, 2-Left, and 3-Right) Binary search algorithm divide the search interval in half, this process makes the maximum number of comparisons (Average case complexity of Search) is O(log2 n) (pronounce this "big-Oh-n" or "the order of magnitude"), if we search in a list consists of (N) elements. …”
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  6. 46

    Simulation of Binary-single Interactions in AGN Disk. I. Gas-enhanced Binary Orbital Hardening by Mengye Wang, Yiqiu Ma, Hui Li, Qingwen Wu, Ya-Ping Li, Xiangli Lei, Jiancheng Wu

    Published 2025-01-01
    “…Stellar-mass binary black hole (BBH) mergers within the accretion disks of active galactic nuclei may contribute to gravitational wave (GW) events detected by ground-based GW detectors. …”
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  7. 47

    Photometric Determination of Unresolved Main-sequence Binaries in the Pleiades: Binary Fraction and Mass-ratio Distribution by Rongrong Liu, Zhengyi Shao, Lu Li

    Published 2025-01-01
    “…This distribution can be interpreted as a fiducial power-law profile with an exponent of −1.0 that is determined in the range of 0.3 < q < 0.8, but with a deficiency of binaries at lower q and an excess at higher q . …”
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  8. 48

    Eccentricities of Close Stellar Binaries by Yanqin Wu, Sam Hadden, Janosz Dewberry, Kareem El-Badry, Christopher D. Matzner

    Published 2025-01-01
    “…Here, we use thousands of main-sequence binaries from the Gaia DR3 catalog to reveal that binaries inward of a few astronomical units exhibit a simple Rayleigh distribution with a mode of σ _e  ≃ 0.3. …”
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    The XRISM/Resolve View of the Fe K Region of Cyg X-3 by XRISM Collaboration, Marc Audard, Hisamitsu Awaki, Ralf Ballhausen, Aya Bamba, Ehud Behar, Rozenn Boissay-Malaquin, Laura Brenneman, Gregory V. Brown, Lia Corrales, Elisa Costantini, Renata Cumbee, María Díaz Trigo, Chris Done, Tadayasu Dotani, Ken Ebisawa, Megan E. Eckart, Dominique Eckert, Satoshi Eguchi, Teruaki Enoto, Yuichiro Ezoe, Adam Foster, Ryuichi Fujimoto, Yutaka Fujita, Yasushi Fukazawa, Kotaro Fukushima, Akihiro Furuzawa, Luigi Gallo, Javier A. García, Liyi Gu, Matteo Guainazzi, Kouichi Hagino, Kenji Hamaguchi, Isamu Hatsukade, Katsuhiro Hayashi, Takayuki Hayashi, Natalie Hell, Edmund Hodges-Kluck, Ann Hornschemeier, Yuto Ichinohe, Manabu Ishida, Kumi Ishikawa, Yoshitaka Ishisaki, Jelle Kaastra, Timothy Kallman, Erin Kara, Satoru Katsuda, Yoshiaki Kanemaru, Richard Kelley, Caroline Kilbourne, Shunji Kitamoto, Shogo Kobayashi, Takayoshi Kohmura, Aya Kubota, Maurice Leutenegger, Michael Loewenstein, Yoshitomo Maeda, Maxim Markevitch, Hironori Matsumoto, Kyoko Matsushita, Dan McCammon, Brian McNamara, François Mernier, Eric D. Miller, Jon M. Miller, Ikuyuki Mitsuishi, Misaki Mizumoto, Tsunefumi Mizuno, Koji Mori, Koji Mukai, Hiroshi Murakami, Richard Mushotzky, Hiroshi Nakajima, Kazuhiro Nakazawa, Jan-Uwe Ness, Kumiko Nobukawa, Masayoshi Nobukawa, Hirofumi Noda, Hirokazu Odaka, Shoji Ogawa, Anna Ogorzalek, Takashi Okajima, Naomi Ota, Stephane Paltani, Robert Petre, Paul Plucinsky, Frederick S. Porter, Katja Pottschmidt, Kosuke Sato, Toshiki Sato, Makoto Sawada, Hiromi Seta, Megumi Shidatsu, Aurora Simionescu, Randall Smith, Hiromasa Suzuki, Andrew Szymkowiak, Hiromitsu Takahashi, Mai Takeo, Toru Tamagawa, Keisuke Tamura, Takaaki Tanaka, Atsushi Tanimoto, Makoto Tashiro, Yukikatsu Terada, Yuichi Terashima, Yohko Tsuboi, Masahiro Tsujimoto, Hiroshi Tsunemi, Takeshi Tsuru, Hiroyuki Uchida, Nagomi Uchida, Yuusuke Uchida, Hideki Uchiyama, Yoshihiro Ueda, Shinichiro Uno, Jacco Vink, Shin Watanabe, Brian J. Williams, Satoshi Yamada, Shinya Yamada, Hiroya Yamaguchi, Kazutaka Yamaoka, Noriko Yamasaki, Makoto Yamauchi, Shigeo Yamauchi, Tahir Yaqoob, Tomokage Yoneyama, Tessei Yoshida, Mihoko Yukita, Irina Zhuravleva, Ryota Tomaru, Tasuku Hayashi, Tomohiro Hakamata, Daiki Miura, Karri Koljonen, Mike McCollough

    Published 2024-01-01
    “…The X-ray binary system Cygnus X-3 (4U 2030+40, V1521 Cyg) is luminous but enigmatic owing to the high intervening absorption. …”
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    Exploring Contact Binaries: Observational Analysis of Four W Uma Binaries Using Photometry and Spectroscopy by A. Panchal, Y. C. Joshi, V. Joshi, A. Chakraborty

    Published 2025-01-01
    “…All the systems except J0805b are A-subtype contact binaries. The absolute parameters of the systems are determined using Gaia DR3 parallax and reddening information. …”
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    Crystallization Properties of Binary Mixtures of Symmetrical Triglycerides 1,3-Dipalmitoyl-2-oleoyl-sn-glycerol (POP) and 1,3-Dioleoyl-2-palmitoyl-sn-glycerol (OPO) by TIAN Xin, CHAI Xiuhang, LIU Yuanfa

    Published 2025-05-01
    Subjects: “…binary mixtures of symmetrical triglycerides 1,3-dipalmitoyl-2-oleoyl-sn-glycerol and 1,3-dioleoyl-2-palmitoyl-sn-glycero; cooling rate; thermodynamic behavior; polymorphism; microstructure…”
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    Evaluation of Color Characteristics, Color Gamut Range and Color Value of Tussah Silk Dyed with Three Natural Dyes and Their Binary Sequential Combination by Fei Xu, Xixian Jia, Zhijun Zhao, Hui Wang, Xinyu Ji

    Published 2025-12-01
    “…The dyed fabrics achieved a color fastness of grade 3 or higher, meeting the standards for daily applications. …”
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    Toward Early-type Eclipsing Binaries as Extragalactic Milestones. IV. Physical Properties of Three Detached O/B-type Systems in the LMC by Mónica Taormina, G. Pietrzyński, R.-P. Kudritzki, B. Pilecki, I. B. Thompson, J. Puls, M. Górski, B. Zgirski, D. Graczyk, M. A. Urbaneja, W. Gieren, W. Narloch, G. Hajdu

    Published 2025-01-01
    “…We present a complete set of physical parameters for three early-type eclipsing binary systems in the Large Magellanic Cloud (LMC): OGLE LMC-ECL-17660, OGLE LMC-ECL-18794, and HV 2274, together with the orbital solutions. …”
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