Works matching DE "HIGH mass stars"
Results: 84
NEW HORIZONS IN BLACK HOLE ASTROPHYSICS.
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- Europhysics News, 2021, v. 52, n. 1, p. 12, doi. 10.1051/epn/2021101
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Dust Temperature Profiles in Dense Cores Related to the High-Mass Star-Forming Regions.
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- Radiophysics & Quantum Electronics, 2022, v. 64, n. 12, p. 857, doi. 10.1007/s11141-022-10184-1
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Formation, Possible Detection and Consequences of Highly Magnetized Compact Stars.
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- Particles (2571-712X), 2022, v. 5, n. 4, p. 493, doi. 10.3390/particles5040037
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A Survey of High-Mass Star Forming Regions in the Line of Singly Deuterated Ammonia NH<sub>2</sub>D.
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- Astronomy Reports, 2024, v. 68, n. 8, p. 771, doi. 10.1134/S1063772924700719
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Investigation of H<sub>2</sub>O and OH Masers in the Region of Formation of a Young High-Mass Stellar Object (S255 NIRS 3).
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- Astronomy Reports, 2024, v. 68, n. 5, p. 453, doi. 10.1134/S1063772924700434
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Time Domain Astronomy Case: Use of Large Photometric Surveys for Study of Variable Stars.
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- Astronomy Reports, 2023, v. 67, n. 9, p. 951, doi. 10.1134/S1063772923090093
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The extended halo and tidal tails of the old open cluster NGC 2112.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 6, p. 1253, doi. 10.1093/pasj/psae085
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ACA CO(J = 2–1) mapping of the nearest spiral galaxy M 33. II. Exploring the evolution of giant molecular clouds.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 5, p. 1098, doi. 10.1093/pasj/psae073
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A kinematic analysis of the giant molecular complex W3: Possible evidence for cloud–cloud collisions that triggered OB star clusters in W3 Main and W3(OH).
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 5, p. 895, doi. 10.1093/pasj/psae056
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High-mass star formation in the Large Magellanic Cloud triggered by colliding H i flows.
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- Publications of the Astronomical Society of Japan, 2024, v. 76, n. 4, p. 589, doi. 10.1093/pasj/psae035
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FUGIN hot core survey. I. Survey method and initial results for l = 10°–20°.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, n. 3, p. 568, doi. 10.1093/pasj/psab021
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CO observations of the molecular gas in the Galactic H ii region Sh2-48: Evidence for cloud–cloud collision as a trigger of high-mass star formation.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psy098
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Cloud–cloud collisions in the common foot point of molecular loops 1 and 2 in the Galactic Center.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psz119
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CO observations toward the isolated mid-infrared bubble S44: External triggering of O-star formation by a cloud–cloud collision.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psy109
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FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). VIII. Possible evidence of cloud–cloud collisions triggering high-mass star formation in the giant molecular cloud M 16 (Eagle Nebula).
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa083
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Rapid and efficient mass collection by a supersonic cloud–cloud collision as a major mechanism of high-mass star formation.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa079
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Triggered high-mass star formation in the H ii region W 28 A2: A cloud–cloud collision scenario.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa054
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ALMA CO observations of a giant molecular cloud in M 33: Evidence for high-mass star formation triggered by cloud–cloud collisions.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa045
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High-mass star formation in Orion B triggered by cloud–cloud collision: Merging molecular clouds in NGC 2024.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa049
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High-mass star formation in Orion possibly triggered by cloud–cloud collision. III. NGC 2068 and NGC 2071.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa005
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Cluster formation induced by a cloud–cloud collision in [DBS2003]179.
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- Publications of the Astronomical Society of Japan, 2021, v. 73, p. 1, doi. 10.1093/pasj/psaa017
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Spin evolution of neutron stars in wind-fed high-mass X-ray binaries.
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- Publications of the Astronomical Society of Japan, 2020, v. 72, n. 6, p. 1, doi. 10.1093/pasj/psaa087
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Observations of 6.7GHz methanol masers with East-Asian VLBI Network. II. Internal proper motion measurement in G006.79-00.25.
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- Publications of the Astronomical Society of Japan, 2016, v. 68, n. 5, p. 1, doi. 10.1093/pasj/psv089
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Charged Spherical Solution in Torsion and Matter Coupling Gravity and Influence of Torsion Parameter and Electric Charge on Compact Stars in Lower Mass Gap.
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- Progress of Theoretical & Experimental Physics: PTEP, 2024, v. 2024, n. 4, p. 1, doi. 10.1093/ptep/ptae043
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Speed of sound and quark confinement inside neutron stars.
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- European Physical Journal: Special Topics, 2020, v. 229, n. 22/23, p. 3651, doi. 10.1140/epjst/e2020-000093-3
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On the age and metallicity of planet-hosting triple star systems.
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- Astrophysics & Space Science, 2024, v. 369, n. 9, p. 1, doi. 10.1007/s10509-024-04351-1
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UV spectropolarimetry with Polstar: protoplanetary disks.
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- Astrophysics & Space Science, 2022, v. 367, n. 12, p. 1, doi. 10.1007/s10509-022-04125-7
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β-decay properties of some astrophysically important Sc isotopes.
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- Astrophysics & Space Science, 2021, v. 366, n. 8, p. 1, doi. 10.1007/s10509-021-03990-y
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Dish on the Cosmos: Resolving the Supergiants.
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- Journal of the Royal Astronomical Society of Canada, 2024, v. 118, n. 1, p. 20
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Galaxies and Starbirth.
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- Journal of the Royal Astronomical Society of Canada, 2022, v. 116, n. 5, p. 193
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A Quenched Galaxy.
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- Journal of the Royal Astronomical Society of Canada, 2021, v. 115, n. 5, p. 221
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Variable Stars I Have Known—And You Should, Too.
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- Journal of the Royal Astronomical Society of Canada, 2021, v. 115, n. 1, p. 46
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Looking Back at the Past Decade.
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- Journal of the Royal Astronomical Society of Canada, 2021, v. 115, n. 1, p. 43
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Three-Component Stäckel Model of the Galaxy Based on the Rotation Curve from Maser Data.
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- Astrophysical Bulletin, 2021, v. 76, n. 2, p. 146, doi. 10.1134/S1990341321020024
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Herbig Stars: A Quarter Century of Progress.
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- Space Science Reviews, 2023, v. 219, n. 1, p. 1, doi. 10.1007/s11214-023-00949-z
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Confirmation and characterization of neglected WDS systems using Gaia data release 3 and the virtual observatory.
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- Astronomische Nachrichten, 2023, v. 344, n. 10, p. 1, doi. 10.1002/asna.20230116
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Astrophysical parameters and dynamical evolution of open clusters: NGC 2587, Collinder 268 and Melotte 72, and Pismis 7.
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- Astronomische Nachrichten, 2021, v. 342, n. 7/8, p. 975, doi. 10.1002/asna.202113983
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Neutron stars in extended scalar-Gauss–Bonnet gravity: the richness of the solution spectrum.
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- European Physical Journal C -- Particles & Fields, 2024, v. 84, n. 12, p. 1, doi. 10.1140/epjc/s10052-024-13704-7
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Metal‐poor stars observed with the automated planet finder telescope. III. CEMP‐no stars are the descendant of population III stars.
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- Astronomische Nachrichten, 2021, v. 342, n. 4, p. 625, doi. 10.1002/asna.202113867
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MASS ACCRETION FLOWS IN THE HIGH-MASS STAR FORMING COMPLEX NGC6334.
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- EAS Publications Series, 2015, v. 75/76, p. 269, doi. 10.1051/eas/1575053
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HOBYS INSIGHTS ON HIGH-MASS STAR FORMATION.
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- EAS Publications Series, 2015, v. 75/76, p. 237, doi. 10.1051/eas/1575047
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HIGH-MASS STAR FORMATION.
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- EAS Publications Series, 2015, v. 75/76, p. 227, doi. 10.1051/eas/1575046
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Protoplanetary disks around young stellar and substellar objects in the σ Orionis cluster.
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- Journal of Astrophysics & Astronomy, 2023, v. 44, n. 2, p. 1, doi. 10.1007/s12036-023-09968-2
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Triggered and dispersed under feedback of super HII region W4.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2025, v. 693, p. 1, doi. 10.1051/0004-6361/202450914
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Properties of intermediate- to high-mass stars in the young cluster M17: Characterizing the (pre-)zero-age main sequence.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450494
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Constraints on the primordial misalignment of star-disk systems.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450410
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Dynamical accretion flows: ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449794
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ALMA-IMF: XV. Core mass function in the high-mass star formation regime.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202345986
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Discovery of a new N-emitter in the epoch of reionization.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202450721
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Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 687, p. 1, doi. 10.1051/0004-6361/202348565
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