Halo Nevi Are Not Trivial: About 2 Young Patients of Regressed Primary Melanoma That Simulates Halo Nevi by S. De Schrijver, I. Theate, O. Vanhooteghem

“…We present two case reports suggesting that a halo nevus appearance can be seen in melanoma, even in young adults. …”
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Reversed Halo Sign in Tuberous Sclerosis Complex by Kazuhiro Suzuki, Kuniaki Seyama, Takuo Hayashi, Yuki Yamashiro, Akihiko Shiraishi, Ryohei Kuwatsuru

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Galactic Halo Wormhole Solutions in f(T) Gravity by M. Sharif, Shamaila Rani

“…The proposal of galactic halo region is based on the idea that dark halos contain some characteristics needed to support traversable wormhole solutions. …”
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Cleaning the beam halo using nonlinear ac magnets by F. Capoani, A. Bazzani, M. Giovannozzi

“…Recently, nonlinear effects have been used to cool a special beam represented by an annular distribution in a 2D phase space. This outcome was accomplished using an ac dipole combined with amplitude detuning generated by static nonlinear magnets. …”
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Dwarf Galaxies in Voids: Dark Matter Halos and Gas Cooling by Matthias Hoeft, Stefan Gottlöber

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Halo-RPD: searching for RNA-binding protein targets in plants by A. O. Shamustakimova

“…A high-affinity substrate has been created to allow covalent binding by chimeric proteins, minimizing protein loss during protein isolation. In this paper, a HaloTag-based method, which we called Halo-RPD (HaloTag RNA PullDown), is presented. …”
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Progenitor Diversity in the Accreted Stellar Halos of Milky Way–like Galaxies by Sy-Yun Pu, Andrew P. Cooper, Robert J. J. Grand, Facundo A. Gómez, Antonela Monachesi

“…We compare, at face value, to current constraints on the radial diversity of the Milky Way's accreted halo. These constraints imply that the halo of our Galaxy is dominated by ∼2 progenitors in the range 8–45 kpc, in contrast to averages of 7 progenitors in the Bullock & Johnston models, 3.5 in Aquarius, and 4.2 in Auriga over the same region. …”
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Asymmetric multi-component trifunctionalization reactions with α-Halo Rh-carbenes by Xiaoyan Yang, Xiaoyu Zhou, Wenhao Hu, Yu Qian

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Refined Modeling of Geoeffective Fast Halo CMEs During Solar Cycle 24 by E. Yordanova, M. Temmer, M. Dumbović, C. Scolini, E. Paouris, A. L. E. Werner, A. P. Dimmock, L. Sorriso‐Valvo

“…This approach resulted in a reduced MAE in the forecast for the arrival time of 8.6 ± 2.2–13.5 ± 2.2 hr and the impact speed of 51 ± 6–243 ± 45 km/s. …”
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Impact of Molecular and Crystal Structure on the Melting Points in Halo-Substituted Phenyl-Quinazolinones by Ivica Đilović, Nenad Judaš, Mario Komar, Maja Molnar, Marta Počkaj, Tomislav Balić

“…Three halo-substituted phenyl-quinazolinone derivatives were prepared and structurally characterized [<b>1</b> = 3-(4-chlorophenyl)-6-iodo-2-methylquinazolin-4(3<i>H</i>)-one, <b>2</b> = 6-iodo-3-(4-methoxyphenyl)-2-methylquinazolin-4(3<i>H</i>)-one, and <b>3</b> = 7-chloro-2-methyl-3-[4-(trifluoromethoxy)phenyl]quinazolin-4(3<i>H</i>)-one)] in order to explore the relationship between structure and melting point in this group of compounds. …”
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Galaxy Evolution in a Pilot Survey up to z=1 and CDM Halos by E. Giraud, J. Melnick, Q.-S. Gu, H. Quintana, F. Selman, I. Toledo, P. Zelaya

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Bose-Einstein Condensate Dark Matter Halos Confronted with Galactic Rotation Curves by M. Dwornik, Z. Keresztes, E. Kun, L. Á. Gergely

“…We present a comparative confrontation of both the Bose-Einstein Condensate (BEC) and the Navarro-Frenk-White (NFW) dark halo models with galactic rotation curves. We employ 6 High Surface Brightness (HSB), 6 Low Surface Brightness (LSB), and 7 dwarf galaxies with rotation curves falling into two classes. …”
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Inner radius and energy conditions of dark matter halos surrounding Schwarzschild black holes by Zibo Shen, Anzhong Wang, Shaoyu Yin

“…We study a class of analytic models for a dark matter halo surrounding a Schwarzschild black hole sitting at the center of a galaxy, with a variable inner radius rin at which the density profile of the dark matter halo vanishes. …”
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Efecto del arreglo espacial de mijo perla en ambientes halo-hidromórficos by Nicolás Bertram, S. Chiacchiera, F.R. Angeletti

“…El objetivo del trabajo fue determinar con qué arreglo espacial se obtiene el mejor establecimiento y acumulación de biomasa de mijo perla en ambientes halo-hidromórficos. Así, durante las etapas de establecimiento temprano (450ºCd) el incremento en la densidad de siembra de mijo perla aumentó la densidad de individuos (plantas.m-2) hasta densidades de 18 kg.ha-1, diluyéndose hacia la primera acumulación (750ºCd) y hallando una meseta en la densidad de macollos con densidades de siembra de 12 kg.ha-1; sin embargo no se halló ninguna diferencia entre las densidades utilizadas en la segunda acumulación (1450ºCd). …”
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Assessing the Dark Matter Content of Two Quasar Host Galaxies at z ∼ 6 through Gas Kinematics by Qinyue Fei, John D. Silverman, Seiji Fujimoto, Ran Wang, Luis C. Ho, Manuela Bischetti, Stefano Carniani, Michele Ginolfi, Gareth Jones, Roberto Maiolino, Wiphu Rujopakarn, N. M. Förster Schreiber, Juan M. Espejo Salcedo, L. L. Lee

“…We conduct a study of the gas kinematics of two quasar host galaxies at z  ≳ 6 traced by the [C ii ] emission line using the Atacama Large Millimeter/submillimeter Array. …”
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Quasinormal modes of Schwarzschild-like black hole surrounded by the pseudo-isothermal dark matter halo by Yanqiang Liu, Benrong Mu, Jun Tao, Yuling Weng

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Analysis of Induced Field in the Brain Tissue by Transcranial Magnetic Stimulation Using Halo-V Assembly Coil by Khaleda Akhter Sathi, Md. Kamal Hosain, Md. Azad Hossain

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Particle motion and QPOs around Euler-Heisenberg black hole immersed in cold dark matter halo by G. Mustafa, S.K. Maurya, Tayyab Naseer, Arzu Cilli, Ertan Güdekli, Assmaa Abd-Elmonem, Neissrien Alhubieshi

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Efecto de la concentración salina y el regimen hídrico sobre la germinación, emergencia y establecimiento de alfalfa (Medicago sativa L.) by N. A. Bertram, C. Alfonso, S. Grande, S. Chiacchiera, A. Ohanian, J. Bonvillani, M.B. Conde, F.R. Angeletti

“…Los suelos halo-hidromórficos de la región húmeda y subhúmeda de Argentina suman aproximadamente 20 millones de hectáreas, un amplio porcentaje de estos presentan vegetación nativa de baja producción de biomasa y consumo de agua. …”
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NEW PYRIDINE-3-SULFONATO TIN (IV), ANTIMONY (III) AND (V) HALO ADDUCTS AND COMPLEXES: SYNTHESIS AND INFRARED STUDY by AÏSSATOU GUEYE, MOUHAMADOU BIRAME DIOP, LIBASSE DIOP

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