Works matching DE "PULSARS"
Results: 1205
ARE SERENDIPITOUS DISCOVERIES A PART OF NORMAL SCIENCE? THE CASE OF THE PULSARS.
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- Sociological Review, 1977, v. 25, n. 1, p. 73, doi. 10.1111/j.1467-954X.1977.tb00279.x
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- Article
Heating of millisecond pulsars by magnetic field decay.
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- Astronomische Nachrichten, 2024, v. 345, n. 5, p. 1, doi. 10.1002/asna.20240032
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- Article
Spin period evolution of Vela pulsar based on the wind emission: Application to the long period radio pulsars GPM J1839‐10 (P = 21 min) and GLEAM‐X J1627 (P = 18 min).
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- Astronomische Nachrichten, 2024, v. 345, n. 5, p. 1, doi. 10.1002/asna.20230176
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- Article
The magnetar crustal magneto‐thermal evolution.
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- Astronomische Nachrichten, 2024, v. 345, n. 2/3, p. 1, doi. 10.1002/asna.20240011
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- Article
Non‐symmetrical sparking may hint "zits" on a pulsar surface.
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- Astronomische Nachrichten, 2024, v. 345, n. 2/3, p. 1, doi. 10.1002/asna.20240010
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- Article
A short review of the pulsar magnetic inclination angles (II).
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- Astronomische Nachrichten, 2024, v. 345, n. 2/3, p. 1, doi. 10.1002/asna.20230167
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Repeating fast radio bursts reveal the secret of pulsar magnetospheric activity.
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- Astronomische Nachrichten, 2024, v. 345, n. 2/3, p. 1, doi. 10.1002/asna.20230153
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A short review on the pulsar magnetic inclination angles.
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- Astronomische Nachrichten, 2023, v. 344, n. 6, p. 1, doi. 10.1002/asna.20220111
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An application of pulsar timing in dynamic reference frame transformation of solar system.
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- Astronomische Nachrichten, 2023, v. 344, n. 3, p. 1, doi. 10.1002/asna.20220026
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The influence of deceleration and internal structure on the braking index of pulsars: Simplest model for the star.
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- Astronomische Nachrichten, 2023, v. 344, n. 1/2, p. 1, doi. 10.1002/asna.20230003
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- Article
Origin of emission in TeV J2032 + 4130 objects of unresolved nature.
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- Astronomische Nachrichten, 2023, v. 344, n. 1/2, p. 1, doi. 10.1002/asna.20220094
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- Article
Generation of cosmic rays in pulsar wind nebulae.
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- Astronomische Nachrichten, 2023, v. 344, n. 1/2, p. 1, doi. 10.1002/asna.20220092
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A list of guest‐star records in Korean history and their possible counterparts.
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- Astronomische Nachrichten, 2022, v. 343, n. 9/10, p. 1, doi. 10.1002/asna.20220017
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The observations of the gigahertz‐peaked spectra pulsars.
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- Astronomische Nachrichten, 2021, v. 342, n. 9/10, p. 1191, doi. 10.1002/asna.20210043
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- Article
The dissipation of toroidal magnetic fields and spin‐down evolution of young and strongly magnetized pulsars.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 369, doi. 10.1002/asna.202113936
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Precession of triaxially deformed neutron stars.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 364, doi. 10.1002/asna.202113935
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Pulsar tests of the graviton mass.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 300, doi. 10.1002/asna.202113923
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Time‐scale analysis of integrated pulse profiles for PSR B0329 + 54.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 283, doi. 10.1002/asna.202113920
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Angular momentum conservation and core superfluid dynamics for the pulsar J1734‐3333.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 255, doi. 10.1002/asna.202113914
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Explaining high braking indices of magnetars SGR 0501+4516 and 1E 2259+586 using the double magnetic‐dipole model.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 249, doi. 10.1002/asna.202113913
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The influence of rotation deceleration on the shape of a pulsar may reflect on the star's braking index.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 222, doi. 10.1002/asna.202113908
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Magnetic field decay in young radio pulsars.
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- Astronomische Nachrichten, 2021, v. 342, n. 1, p. 216, doi. 10.1002/asna.202113907
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Spectral energy distribution modeling of broadband emission in the pulsar wind nebula 3C 58.
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- Astronomische Nachrichten, 2020, v. 341, n. 2, p. 170, doi. 10.1002/asna.202023774
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A hybrid model for pulsar's spin‐down evolution.
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- Astronomische Nachrichten, 2019, v. 340, n. 9/10, p. 1035, doi. 10.1002/asna.201913712
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The evolution of magnetic field and spin‐down of young pulsars.
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- Astronomische Nachrichten, 2019, v. 340, n. 9/10, p. 1023, doi. 10.1002/asna.201913710
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The study of coherent optical pulsations of the millisecond pulsar PSR J1023+0038 on Russian 6‐m telescope.
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- Astronomische Nachrichten, 2019, v. 340, n. 7, p. 607, doi. 10.1002/asna.201913663
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On the connection between radiative outbursts and timing irregularities in magnetars.
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- Astronomische Nachrichten, 2019, v. 340, n. 4, p. 340, doi. 10.1002/asna.201913621
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Constraints on the number of X‐ray pulsars in IC 10 from a deep XMM‐Newton observation.
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- Astronomische Nachrichten, 2019, v. 340, n. 1-3, p. 62, doi. 10.1002/asna.201913561
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Evolution of high‐mass X‐ray binaries in the small magellanic cloud.
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- Astronomische Nachrichten, 2019, v. 340, n. 1-3, p. 46, doi. 10.1002/asna.201913557
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The radial and rotational velocity of ζ Ophiuchi.
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- Astronomische Nachrichten, 2018, v. 339, n. 1, p. 46, doi. 10.1002/asna.201713383
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Heavier and darker.
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- Astronomische Nachrichten, 2017, v. 338, n. 9/10, p. 1034, doi. 10.1002/asna.201713430
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Contents: Astron. Nachr. 9-10/2017.
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- Astronomische Nachrichten, 2017, v. 338, n. 9/10, p. 963, doi. 10.1002/asna.201705008
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- Article
Could the low-braking-index pulsar PSR J1734-3333 evolve into a magnetar?
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- Astronomische Nachrichten, 2017, v. 338, n. 9/10, p. 1060, doi. 10.1002/asna.201713436
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Cover Picture: Astron. Nachr. 8-9/2015.
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- 2015
- Publication type:
- Editorial
An effective field theory for neutron stars with many-body forces, strong ∑<sup>-</sup> repulsion, and K<sup>-</sup> and $\bar K^0$ condensation.
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- Astronomische Nachrichten, 2015, v. 336, n. 8/9, p. 880, doi. 10.1002/asna.201512242
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Magnetic field decay in normal radio pulsars.
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- Astronomische Nachrichten, 2015, v. 336, n. 8/9, p. 831, doi. 10.1002/asna.201512232
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Ultraluminous X-ray pulsar: Accreting magnetar?
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- Astronomische Nachrichten, 2015, v. 336, n. 8/9, p. 835, doi. 10.1002/asna.201512233
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Magneto-rotational and thermal evolution of young neutron stars.
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- 2015
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- Editorial
Interplanetary GPS using pulsar signals.
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- 2015
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- Editorial
3XMM J185246.6+003317 as transient neutron star.
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- Astronomische Nachrichten, 2015, v. 336, n. 6, p. 545, doi. 10.1002/asna.201412189
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- Article
A millisecond pulsar position determined to 0.2 mas precision with VLBI.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451492
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Eccentricity effects on the supermassive black hole gravitational wave background.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202451345
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Beyond the Hellings–Downs curve: Non-Einsteinian gravitational waves in pulsar timing array correlations.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 691, p. 1, doi. 10.1051/0004-6361/202449483
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Short-term variability of the transitional pulsar candidate CXOU J110926.4−650224 from X-rays to infrared.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450915
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Two black widow pulsars in the optical and X-rays.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450205
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Comparison of the disk precession models with the photometric behavior of TT Ari in 2021-2023.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202450042
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Bayesian sensitivity of binary pulsars to ultra-light dark matter.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449953
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Revisiting thermoelectric effects in the crust of neutron stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449692
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Multiwavelength identification of millisecond pulsar candidates in the Galactic bulge.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449473
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High-temporal-resolution optical spectroscopic observations of the transitional millisecond pulsar PSR J1023+0038.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2024, v. 690, p. 1, doi. 10.1051/0004-6361/202449466
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- Article