The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays (2018)
- Authors:
- Autor USP: PINO, ELISABETE MARIA DE GOUVEIA DAL - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/sty1499
- Assunto: RAIOS X
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 479, p. 1672-1684, 2018
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
KUSHWAHA, Pankaj et al. The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays. Monthly Notices of the Royal Astronomical Society, v. 479, p. 1672-1684, 2018Tradução . . Disponível em: https://doi.org/10.1093/mnras/sty1499. Acesso em: 19 jan. 2026. -
APA
Kushwaha, P., Gupta, A. C., Wiita, P. J., Pal, M., Gaur, H., & Dal Pino, E. M. de G. (2018). The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays. Monthly Notices of the Royal Astronomical Society, 479, 1672-1684. doi:10.1093/mnras/sty1499 -
NLM
Kushwaha P, Gupta AC, Wiita PJ, Pal M, Gaur H, Dal Pino EM de G. The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 479 1672-1684.[citado 2026 jan. 19 ] Available from: https://doi.org/10.1093/mnras/sty1499 -
Vancouver
Kushwaha P, Gupta AC, Wiita PJ, Pal M, Gaur H, Dal Pino EM de G. The ever-surprising blazar OJ 287: multiwavelength study and appearance of a new component in X-rays [Internet]. Monthly Notices of the Royal Astronomical Society. 2018 ; 479 1672-1684.[citado 2026 jan. 19 ] Available from: https://doi.org/10.1093/mnras/sty1499 - Simulações magnetohidrodinâmicas de reconexões magnéticas em disco de acreção
- Disc formation in turbulent cloud cores: is magnetic flux loss necessary to stop the magnetic braking catastrophe or not?
- Multiwavelength temporal and spectral variability of the blazar OJ 287 during and after the 2015 December flare: a major accretion disc contribution
- Erratum: The role of fast magnetic reconnection on the radio and gamma-ray emission from the nuclear regions of microquasars and Low luminosity AGNs
- Are tachoclines important for solar and stellar dynamos?: What can we learn from global simulations
- Particle acceleration by magnetic reconnection in accretion disk/jet systems
- Jet-ISM cloud interactions: 3D simulations of the HH 270/110 jet system
- Turbulent pumping in solar dynamo models
- Cosmic magnetic fields: from stars and galaxies to the primordial Universe
- Supernova explosions and the triggering of galactic fountains and outflows
Informações sobre o DOI: 10.1093/mnras/sty1499 (Fonte: oaDOI API)
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