The magnetic field in the central parsec by Glasse, A, Aitken, D, Roche, P

An Updated Reference Frame for the Galactic Inner Parsec by Jeremy Darling, Jennie Paine, Mark J. Reid, Karl M. Menten, Shoko Sakai, Andrea Ghez

“…Infrared observations of stellar orbits about Sgr A* probe the mass distribution in the inner parsec of the Galaxy and provide definitive evidence for the existence of a massive black hole. …”
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Galactic star formation in parsec-scale resolution simulations by Powell, L, Bournaud, F, Chapon, D, Devriendt, J, Slyz, A, Teyssier, R

“…We investigate how star formation (SF) proceeds in simulated galaxies when we obtain parsec-scale resolution and more successfully capture the multiphase ISM. …”

Evolution of Magnetic Field of the Quasar 1604+159 at parsec Scale by Xu-Zhi Hu, Xiaoyu Hong, Wei Zhao, Liang Chen, Wei-Yang Wang, Linhui Wu

“…We have analyzed the total intensity, spectral index, linear polarization, and rotation measure (RM) distributions at the parsec scale for the quasar 1604+159. The source was observed at 5.0, 8.4, and 15.4 GHz in 2002 and 4.6, 5.1, 6.0, 7.8, 12.2, 15.2, and 43.9 GHz in 2020 with the American Very Long Baseline Array (VLBA). …”
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High resolution imaging of the magnetic field in the central parsec of the Galaxy by Roche, P, Lopez Rodriguez, E, Telesco, C, Schodel, R, Packham, C

Optimizing NACA2414 airfoil aerodynamics with PARSEC parametrization and Genetic Algorithm by Krishnan Anupam, Al-Obaidi Abdulkareem Sh. Mahdi, Ching Hao Lee

“…The study explores the airfoil’s performance across a range of -10 to 15 degrees angle of attack. It employs both PARSEC parametrization and Genetic Algorithm optimization, achieving significant advancements. …”
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Inflation of 430-parsec bipolar radio bubbles in the Galactic Centre by an energetic event by Heywood, I, Camilo, F, Cotton, WD, Yusef-Zadeh, F, Abbott, TD, RM Adam, MA Aldera, EF Bauermeister, RS Booth, AG Botha, DH Botha, LRS Brederode, ZB Brits, SJ Buchner, JP Burger, JM Chalmers, T Cheetham, D de Villiers, MA Dikgale-Mahlakoana, LJ du Toit, SWP Esterhuyse, BL Fanaroff, AR Foley, DJ Fourie, RRG Gamatham, S Goedhart, S Gounden, MJ Hlakola, CJ Hoek, A Hokwana, DM Horn, JMG Horrell, B Hugo, AR Isaacson, JL Jonas, JDBL Jordaan, AF Joubert, GIG Józsa, RPM Julie, FB Kapp, JS Kenyon, PPA Kotzé, H Kriel, TW Kusel, R Lehmensiek, D Liebenberg, A Loots, RT Lord, BM Lunsky, PS Macfarlane

“…Here we report radio imaging that reveals a bipolar bubble structure, with an overall span of 1 degree by 3 degrees (140 parsecs × 430 parsecs), extending above and below the Galactic plane and apparently associated with the Galactic Centre. …”

REPRESENTATION METHOD EFFECTS ON VIBRATIONAL GENETIC ALGORITHM IN 2-D AIRFOIL DESIGN by Y. Volkan Pehlivanoglu

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The Accretion Mode in Sub-Eddington Supermassive Black Holes: Getting into the Central Parsecs of Andromeda by C. Alig, A. Prieto, M. Blaña, M. Frischman, C. Metzl, A. Burkert, O. Zier, A. Streblyanska

“…The evolution of a streamer of gas particles moving under the barred potential of M31 is followed from kiloparsec distance to the central parsecs. After an exploratory study of initial conditions, a compelling fit to the observed dust/ionized gas morphologies and line-of-sight velocities in the inner hundreds of parsecs is produced. …”
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Mid-infrared polarization studies of SgrA: a three-dimensional study of the central parsec by Aitken, D, Smith, C, Moore, T, Roche, P

“…It is shown that the physical conditions in the ionized filaments of the central parsec lead to a very uniform grain alignment that is directed along the local magnetic field. …”

X-Ray Polarimetry Reveals the Magnetic-field Topology on Sub-parsec Scales in Tycho’s Supernova Remnant by Riccardo Ferrazzoli, Patrick Slane, Dmitry Prokhorov, Ping Zhou, Jacco Vink, Niccolò Bucciantini, Enrico Costa, Niccolò Di Lalla, Alessandro Di Marco, Paolo Soffitta, Martin C. Weisskopf, Kazunori Asakura, Luca Baldini, Jeremy Heyl, Philip E. Kaaret, Frédéric Marin, Tsunefumi Mizuno, C.-Y. Ng, Melissa Pesce-Rollins, Stefano Silvestri, Carmelo Sgrò, Douglas A. Swartz, Toru Tamagawa, Yi-Jung Yang, Iván Agudo, Lucio A. Antonelli, Matteo Bachetti, Wayne H. Baumgartner, Ronaldo Bellazzini, Stefano Bianchi, Stephen D. Bongiorno, Raffaella Bonino, Alessandro Brez, Fiamma Capitanio, Simone Castellano, Elisabetta Cavazzuti, Chien-Ting Chen, Stefano Ciprini, Alessandra De Rosa, Ettore Del Monte, Laura Di Gesu, Immacolata Donnarumma, Victor Doroshenko, Michal Dovčiak, Steven R. Ehlert, Teruaki Enoto, Yuri Evangelista, Sergio Fabiani, Javier A. Garcia, Shuichi Gunji, Kiyoshi Hayashida, Wataru Iwakiri, Svetlana G. Jorstad, Fabian Kislat, Vladimir Karas, Takao Kitaguchi, Jeffery J. Kolodziejczak, Henric Krawczynski, Fabio La Monaca, Luca Latronico, Ioannis Liodakis, Simone Maldera, Alberto Manfreda, Andrea Marinucci, Alan P. Marscher, Herman L. Marshall, Giorgio Matt, Ikuyuki Mitsuishi, Fabio Muleri, Michela Negro, Stephen L. O’Dell, Nicola Omodei, Chiara Oppedisano, Alessandro Papitto, George G. Pavlov, Abel L. Peirson, Matteo Perri, Pierre-Olivier Petrucci, Maura Pilia, Andrea Possenti, Juri Poutanen, Simonetta Puccetti, Brian D. Ramsey, John Rankin, Ajay Ratheesh, Oliver Roberts, Roger W. Romani, Gloria Spandre, Fabrizio Tavecchio, Roberto Taverna, Yuzuru Tawara, Allyn F. Tennant, Nicholas E. Thomas, Francesco Tombesi, Alessio Trois, Sergey S. Tsygankov, Roberto Turolla, Kinwah Wu, Fei Xie, Silvia Zane

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The central parsecs of Centaurus A: High Excitation Gas, a Molecular Disk, and the Mass of the Black Hole by Neumayer, N, Cappellari, M, Reunanen, J, Rix, H, Werf, P, Zeeuw, P, Davies, R

Unveiling the Solution to the Final-parsec Problem by Combining Millihertz Gravitational-wave Observation and Active Galactic Nucleus Survey by Liang-Gui Zhu, Xian Chen

“…Massive black hole binaries (MBHBs) could be the loudest gravitational-wave (GW) sources in the millihertz (mHz) GW band, but their dynamical evolution may stall when the black holes reach the innermost parsec of a galaxy. Such a “final-parsec problem” could be solved if an MBHB forms in a gas-rich environment, such as an active galactic nucleus (AGN), but other solutions not involving AGNs also exist. …”
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A Large Jet Narrow-line Seyfert 1 Galaxy: Observations from Parsec to 100 kpc Scales by Sina Chen, Preeti Kharb, Silpa Sasikumar, Sumana Nandi, Marco Berton, Emilia Järvelä, Ari Laor, Ehud Behar, Luigi Foschini, Amelia Vietri, Minfeng Gu, Giovanni La Mura, Luca Crepaldi, Minhua Zhou

“…Future radio observations can explore the jet structure between the parsec and 100 kpc scales, the origin of their direction mismatch, and the parsec-scale jet proper motion. …”
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Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81 by Wu Jiang, Zhiqiang Shen, Ivan Martí-Vidal, Zhen Yan, Lei Huang, Roman Gold, Ya-Ping Li, Fuguo Xie, Noriyuki Kawaguchi

“…Studying a centi-parsec supermassive black hole binary (SMBHB) would allow us to explore a new parameter space in active galactic nuclei, and these objects are also potential sources of gravitational waves. …”
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Warm Molecular Gas in the Central Parsecs of the Buried Nucleus of NGC 4418 Traced with the Fundamental CO Rovibrational Absorptions by Youichi Ohyama, Shusuke Onishi, Takao Nakagawa, Kosei Matsumoto, Naoki Isobe, Mai Shirahata, Shunsuke Baba, Kazushi Sakamoto

“…We modeled that the warm CO absorber almost covers the central heating source and that it is an inner layer around the 5 μ m photosphere (at r = several parsecs) of a compact shroud of gas and dust ( d ∼ 100 pc). …”
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Unveiling the central parsec region of an active galactic nucleus: The circinus nucleus in the near-infrared with the very large telescope by Almudhna Prieto, M, Meisenheimer, K, Marco, O, Reunanen, J, Contini, M, Clenet, Y, Davies, R, Gratadour, D, Henning, T, Klaas, U, Kotitanien, J, Leinert, C, Lutz, D, Rouan, D, Thatte, N

“…VLT J- to M'-band adaptive optics observations of the Circinus galaxy on parsec scales resolve a central bright Ks-band source with a FWHM size of 1.9 ± 0.6 pc. …”

Revealing the Intermediate Mass Black Hole at the Heart of Dwarf Galaxy NGC404 with Sub-parsec Resolution ALMA Observations by Bureau, M, Cappellari, M, Liu, L, Smith, MD

Multiphase Gas Nature in the Sub-parsec Region of the Active Galactic Nuclei. I. Dynamical Structures of Dusty and Dust-free Outflow by Yuki Kudoh, Keiichi Wada, Nozomu Kawakatu, Mariko Nomura

“…The dusty outflow from the sub-parsec region can be also a source of material for the radiation-driven fountain for a larger scale.…”
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A Parsec-scale Catalog of Molecular Clouds in the Solar Neighborhood Based on 3D Dust Mapping: Implications for the Mass–Size Relation by Shlomo Cahlon, Catherine Zucker, Alyssa Goodman, Charles Lada, João Alves

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