Works matching Stars
Results: 5000
STAR PROJECTIVE AND STAR INJECTIVE H<sub>v</sub>-MODULES.
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- Journal of the Indonesian Mathematical Society, 2018, v. 24, n. 1, p. 79, doi. 10.22342/jims.24.1.490.79-94
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Magnetic Star-Disk Interaction in Classical T Tauri Stars.
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- Astrophysics & Space Science, 2004, v. 292, n. 1-4, p. 599
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Resolving the Issue of Artefact Deposition at Star Carr.
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- Proceedings of the Prehistoric Society, 2017, v. 83, p. 23, doi. 10.1017/ppr.2017.8
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Pre-main sequence stars, emission stars and recent star formation in the Cygnus region.
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- Bulletin of the Astronomical Society of India, 2007, v. 35, n. 3, p. 383
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Turbulence modelling in neutron star merger simulations: Turbulence modelling in neutron star merger simulations: D. Radice, I. Hawke.
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- Living Reviews in Computational Astrophysics, 2024, v. 10, n. 1, p. 1, doi. 10.1007/s41115-023-00019-9
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The Role of Binary Stars in Understanding the Physics and Evolution of Stars.
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- Astronomy Reports, 2023, v. 67, n. 9, p. 867, doi. 10.1134/S1063772923090135
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Classical Be stars: Rapidly rotating B stars with viscous Keplerian decretion disks.
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- Astronomy & Astrophysics Review, 2013, v. 21, n. 1, p. 1, doi. 10.1007/s00159-013-0069-0
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Methods for relativistic self-gravitating fluids: from binary neutron stars to black hole-disks and magnetized rotating neutron stars.
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- General Relativity & Gravitation, 2022, v. 54, n. 6, p. 1, doi. 10.1007/s10714-022-02928-1
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The properties of a large sample of OH/IR stars, S stars and C-rich AGB stars.
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- Astrophysics & Space Science, 2010, v. 330, n. 1, p. 23, doi. 10.1007/s10509-010-0352-8
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Star cluster formation and star formation: the role of environment and star-formation efficiencies.
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- Astrophysics & Space Science, 2009, v. 324, n. 2-4, p. 129, doi. 10.1007/s10509-009-0088-5
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AGB star intershell abundances inferred from UV spectra of extremely hot post-AGB stars.
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- Astrophysics & Space Science, 2008, v. 320, n. 1-3, p. 159, doi. 10.1007/s10509-008-9911-7
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Effect of Coriolis force on the shapes of rotating stars and stars in binary systems.
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- Astrophysics & Space Science, 2008, v. 319, n. 1, p. 45, doi. 10.1007/s10509-008-9946-9
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Abundances from Disentangled Component Spectra of Close Binary Stars: An Observational Test of an Early Mixing in High-Mass Stars.
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- Astrophysics & Space Science, 2006, v. 304, n. 1-4, p. 329, doi. 10.1007/s10509-006-9151-7
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Investigation of Faint Galactic Carbon Stars from the First Byurakan Spectral sky Survey. Optical Variability. I. N-Type AGB Carbon Stars. K-band Absolute Magnitudes and Distances.
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- Astrophysics, 2014, v. 57, n. 4, p. 510, doi. 10.1007/s10511-014-9354-5
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Microvariability and fast variability of stars. I. standard stars.
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- Astrophysics, 2010, v. 53, n. 4, p. 511, doi. 10.1007/s10511-010-9143-8
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Search for HH-objects and emission stars in star formation regions. VI. Herbig-Haro objects and emission stars in the region of the GM 1-64 and GM 2-4 nebulae.
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- Astrophysics, 2009, v. 52, n. 4, p. 501, doi. 10.1007/s10511-009-9085-1
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Effect of the star limb darkening law on the probabilities of discovering detached close binary stars as eclipsing variables.
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- Astrophysics, 2006, v. 49, n. 1, p. 131, doi. 10.1007/s10511-006-0014-2
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Thermal Support and Rapid Uniform Rotation: Implications on Protoneutron Stars, Hot Neutron Stars, and Neutron Star Merger Remnants.
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- Bulgarian Journal of Physics, 2021, v. 48, n. 5/6, p. 547, doi. 10.55318/bgjp.2021.48.5-6.547
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DOĞRUSAL OLMAYAN MODELLER: TÜRKİYE İÇİN ENFLASYONUN STAR MODELLEMESİ.
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- Journal of Financial Politic & Economic Reviews / Finans Politik & Ekonomik Yorumlar, 2019, v. 56, n. 648, p. 181
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Super-Fast Line-Profile Variability in the Spectra of OBA Stars. II. A0 Star α<sup>2</sup> CVn.
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- Astrophysical Bulletin, 2020, v. 75, n. 3, p. 278, doi. 10.1134/S1990341320030074
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Stars with discrepant v sin i as derived from the Ca II λ3933 Å and Mg II λ4481 Å lines. V. HD 182255 and HD 214923-SPB stars in binary systems.
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- Astrophysical Bulletin, 2016, v. 71, n. 2, p. 199, doi. 10.1134/S1990341316020073
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Stars with discrepant <i>v</i> sin <i>i</i> as derived from the Ca II <i>λ</i>3933 Å and Mg II <i>λ</i>4481 Å lines. IV. HD8837—a shell star, HD47964 and HD183986—new binaries.
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- Astrophysical Bulletin, 2013, v. 68, n. 4, p. 442, doi. 10.1134/S1990341313040056
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Spectroscopy of B and Be Stars in the Very Young Open Star Cluster IC 1805.
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- Astronomy Letters, 2024, v. 50, n. 4, p. 249, doi. 10.1134/S1063773724700142
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Spectroscopy of B and Be Stars in the Young Open Star Cluster NGC 581 (M 103).
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- Astronomy Letters, 2020, v. 46, n. 7, p. 473, doi. 10.1134/S1063773720070087
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Relative content of Be stars in young open star clusters.
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- Astronomy Letters, 2012, v. 38, n. 7, p. 428, doi. 10.1134/S1063773712060059
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Comparison of integrated photometric parameters of extragalactic star formation complexes and open star clusters in the Milky Way.
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- Astronomy Letters, 2009, v. 35, n. 10, p. 679, doi. 10.1134/S1063773709100041
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Kinematic Parameters of the Galactic Spiral Pattern from Data on Open Star Clusters and OB Stars.
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- Astronomy Letters, 2005, v. 31, n. 10, p. 663, doi. 10.1134/1.2075308
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A New Simplified Selection Algorithm of the Guide Star Catalogue for a Star Sensor.
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- Journal of Navigation, 2014, v. 67, n. 6, p. 984, doi. 10.1017/S0373463314000411
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Conversion of neutron stars to 2 + 1 flavor Nambu Jona-Lasinio quark stars as a mechanism for gamma-ray bursts.
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- Modern Physics Letters A, 2017, v. 32, n. 37, p. 1, doi. 10.1142/S0217732317502091
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Gamma-ray bursts generated from phase transition of neutron stars to quark stars.
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- Modern Physics Letters A, 2017, v. 32, n. 4, p. -1, doi. 10.1142/S0217732317500274
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A Robust High-Accuracy Star Map Matching Algorithm for Dense Star Scenes.
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- Remote Sensing, 2024, v. 16, n. 11, p. 2035, doi. 10.3390/rs16112035
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Guide Star Selection for the Three-FOV Daytime Star Sensor.
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- Sensors (14248220), 2019, v. 19, n. 6, p. 1457, doi. 10.3390/s19061457
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Detection of a centrifugal magnetosphere in one of the most massive stars in the ρ Oph star‐forming cloud.
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- Astronomische Nachrichten, 2018, v. 339, n. 1, p. 72, doi. 10.1002/asna.201713457
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A star identification algorithm based on a voting scheme for star trackers.
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- Iranian Journal of Physics Research, 2014, v. 14, n. 1, p. 10
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Proton ingestion in asymptotic giant branch stars as a possible explanation for J-type stars and AB2 grains.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451013
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Massive star cluster formation: II. Runaway stars as fossils of subcluster mergers.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450774
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EWOCS-II: X-ray properties of the Wolf–Rayet stars in the young Galactic super star cluster Westerlund 1.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202348914
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Massive star cluster formation: I. High star formation efficiency while resolving feedback of individual stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202348840
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Contribution of very massive stars to the sulfur abundance in star-forming galaxies: Role of pair-instability supernovae.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202348231
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Disk Evolution Study Through Imaging of Nearby Young Stars (DESTINYS): The SPHERE view of the Orion star-forming region.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 685, p. 1, doi. 10.1051/0004-6361/202347452
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Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS: I. Asteroseismic distances to 12 500 red-giant stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202346196
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Gaia-ESO survey: Massive stars in the Carina Nebula: I. A new census of OB stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 671, p. 1, doi. 10.1051/0004-6361/202245335
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VVVX Near-IR Photometry for 99 Low-mass Stars in the Gaia EDR3 Catalog of Nearby Stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2022, v. 660, p. 1, doi. 10.1051/0004-6361/202141759
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Tomography of cool giant and supergiant star atmospheres: III. Validation of the method on VLTI/AMBER observations of the Mira star S Ori.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038581
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Cool stars in the Galactic center as seen by APOGEE: M giants, AGB stars, and supergiant stars and candidates.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038327
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Unifying low- and high-mass star formation through density-amplified hubs of filaments: The highest mass stars (>100 M<sub>⊙</sub>) form only in hubs.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 642, p. 1, doi. 10.1051/0004-6361/202038232
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Discovery of technetium- and niobium-rich S stars: The case for bitrinsic stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2020, v. 635, p. 1, doi. 10.1051/0004-6361/202037481
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The HST Key Project galaxies NGC 1326A, NGC 1425, and NGC 4548: New variable stars and massive star population.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201936074
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Star formation activity and the spatial distribution and mass segregation of dense cores in the early phases of star formation.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 629, p. 1, doi. 10.1051/0004-6361/201834080
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Masses and ages for metal-poor stars: A pilot programme combining asteroseismology and high-resolution spectroscopic follow-up of RAVE halo stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2019, v. 627, p. 1, doi. 10.1051/0004-6361/201834081
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