Références vérifiées

Références

• snider2020 · Room-temperature superconductivity in a carbonaceous sulfur hydride · 10.1038/s41586-020-2801-z

  Rétracté Cet article a été rétracté. Retirez-le, ou citez-le comme rétracté. Avis de rétractation
  Correction publiée Une correction de cet article a été publiée : vérifiez qu’elle ne change pas ce que vous citez. Correction
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• kral2017 · Predictions for the secondary CO, C and O gas content of debris discs from the destruction of volatile-rich planetesimals · 10.1093/mnras/stx730

  Référence à corriger Notice retrouvée dans Crossref

  • Année : 2016 → 2017
  Correction proposée — à relire avant utilisation

  Votre entrée

  @article{kral2017,
    title={Predictions for the secondary CO, C and O gas content of debris discs from the destruction of volatile-rich planetesimals},
    author={Kral, Quentin and Matr{\`a}, Luca and Wyatt, Mark C. and Kennedy, Grant M.},
    journal={Monthly Notices of the Royal Astronomical Society},
    volume={469},
    pages={521--550},
    year={2016}
  }

  Corrigée

  @article{kral2017,
    title = {Predictions for the secondary CO, C and O gas content of debris discs from the destruction of volatile-rich planetesimals},
    author = {Kral, Quentin and Matr{\`a}, Luca and Wyatt, Mark C. and Kennedy, Grant M.},
    journal = {Monthly Notices of the Royal Astronomical Society},
    volume = {469},
    pages = {521--550},
    year = {2017},
    doi = {10.1093/mnras/stx730},
  }

  Garder cette correction dans le .bib téléchargé

• kral2017b · Predictions for the secondary CO, C and O gas content of debris discs from the destruction of volatile-rich planetesimals · 10.1093/mnras/stx730

  Doublon Le même article que kral2017.
  Entrée incomplète Ajouté d’après la notice qui l’identifie : volume = 469, pages = 521-550.
  Correction proposée — à relire avant utilisation

  Votre entrée

  @article{kral2017b,
    title={Predictions for the secondary CO, C and O gas content of debris discs from the destruction of volatile-rich planetesimals},
    author={Kral, Q. and Matra, L. and Wyatt, M. C. and Kennedy, G. M.},
    journal={MNRAS},
    year={2017},
    doi={10.1093/mnras/stx730}
  }

  Corrigée

  @article{kral2017b,
    title = {Predictions for the secondary CO, C and O gas content of debris discs from the destruction of volatile-rich planetesimals},
    author = {Kral, Q. and Matra, L. and Wyatt, M. C. and Kennedy, G. M.},
    journal = {MNRAS},
    year = {2017},
    doi = {10.1093/mnras/stx730},
    volume = {469},
    pages = {521-550},
  }

  Garder cette correction dans le .bib téléchargé

• eht2022 · First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way · arXiv:2311.08680

  Publication finale disponible Cité comme preprint, mais publié dans The Astrophysical Journal Letters. 10.3847/2041-8213/ac6674
  Correction proposée — à relire avant utilisation

  Votre entrée

  @misc{eht2022,
    title={First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way},
    author={{Event Horizon Telescope Collaboration}},
    year={2023},
    eprint={2311.08680},
    archivePrefix={arXiv}
  }

  Corrigée

  @article{eht2022,
    title = {First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way},
    author = {{Event Horizon Telescope Collaboration}},
    year = {2022},
    eprint = {2311.08680},
    journal = {The Astrophysical Journal Letters},
    volume = {930},
    pages = {L12},
    doi = {10.3847/2041-8213/ac6674},
  }

  Garder cette correction dans le .bib téléchargé

• marino2016 · Exocometary gas in the HD 181327 debris ring · 10.1093/mnras/stw1216

  Entrée incomplète Ajouté d’après la notice qui l’identifie : doi = 10.1093/mnras/stw1216, volume = 460, pages = 2933-2944.
  Correction proposée — à relire avant utilisation

  Votre entrée

  @article{marino2016,
    title={Exocometary gas in the HD 181327 debris ring},
    author={Marino, S. and Matr{\`a}, L. and Stark, C. and Wyatt, M. C. and Casassus, S. and Kennedy, G. and Rodriguez, D. and Zuckerman, B. and Perez, S. and Dent, W. R. F. and Kuchner, M. and Hughes, A. M. and Schneider, G. and Steele, A. and Roberge, A. and Donaldson, J. and Nesvold, E.},
    journal={Monthly Notices of the Royal Astronomical Society},
    year={2016}
  }

  Corrigée

  @article{marino2016,
    title = {Exocometary gas in the HD 181327 debris ring},
    author = {Marino, S. and Matr{\`a}, L. and Stark, C. and Wyatt, M. C. and Casassus, S. and Kennedy, G. and Rodriguez, D. and Zuckerman, B. and Perez, S. and Dent, W. R. F. and Kuchner, M. and Hughes, A. M. and Schneider, G. and Steele, A. and Roberge, A. and Donaldson, J. and Nesvold, E.},
    journal = {Monthly Notices of the Royal Astronomical Society},
    year = {2016},
    doi = {10.1093/mnras/stw1216},
    volume = {460},
    pages = {2933-2944},
  }

  Garder cette correction dans le .bib téléchargé

Citations à vérifier

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• L’article dit autre chose cité pour un résultat · main.tex, ligne 15

  The shadow of the supermassive black hole at the centre of the Milky Way was first imaged with ALMA alone [eht2022].

  The paper attributes the observations to a global array of eight telescopes, not ALMA alone.

  These observations were conducted in 2017 using a global interferometric array of eight telescopes operating at a wavelength of λ = 1.3 mm.

  eht2022

  eht2022 · First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way

  Résumé scientifique

  We present the first Event Horizon Telescope (EHT) observations of Sagittarius A* (Sgr A$^*$), the Galactic center source associated with a supermassive black hole. These observations were conducted in 2017 using a global interferometric array of eight telescopes operating at a wavelength of $λ=1.3\,{\rm mm}$. The EHT data resolve a compact emission region with intrahour variability. A variety of imaging and modeling analyses all support an image that is dominated by a bright, thick ring with a diameter of $51.8 \pm 2.3$\,\uas (68\% credible interval). The ring has modest azimuthal brightness asymmetry and a comparatively dim interior. Using a large suite of numerical simulations, we demonstrate that the EHT images of Sgr A$^*$ are consistent with the expected appearance of a Kerr black hole with mass ${\sim}4 \times 10^6\,{\rm M}_\odot$, which is inferred to exist at this location based on previous infrared observations of individual stellar orbits as well as maser proper motion studies. Our model comparisons disfavor scenarios where the black hole is viewed at high inclination ($i > 50^\circ$), as well as non-spinning black holes and those with retrograde accretion disks. Our results provide direct evidence for the presence of a supermassive black hole at the center of the Milky Way galaxy, and for the first time we connect the predictions from dynamical measurements of stellar orbits on scales of $10^3-10^5$ gravitational radii to event horizon-scale images and variability