Quasar microlensing: Revolutionizing our understanding of quasar structure and dynamics

Bibcode
2019BAAS...51c.487M
Moustakas, Leonidas; Anguita, Timo; Chartas, George; Cornachione, Matthew; Dai, Xinyu; Fian, Carina; Jimenez-Vicente, Jorge; Labrie, Kathleen; Macleod, Chelsea; Mediavilla, Evencio; Morgan, Christopher W.; O'Dowd, Matthew; Lewis, Geraint; Motta, Veronica; Nierenberg, Anna; Pooley, David; Rojas, Karina; Sluse, Dominique; Vernardos, Georgios; Webster, Rachel; Yong, Suk Yee
Referencia bibliográfica

Astro2020: Decadal Survey on Astronomy and Astrophysics, science white papers, no. 487; Bulletin of the American Astronomical Society, Vol. 51, Issue 3, id. 487 (2019)

Advertised on:
5
2019
Número de autores
21
Número de autores del IAC
2
Número de citas
0
Número de citas referidas
0
Descripción
Microlensing in strong-lens systems with quasars provides a unique detailed view of the internal structure of active black holes to the scale of nano- arcseconds. The case is made for the potential of this approach to revolutionize our understanding of quasar physics and its role in broader questions, with a coherent community strategy.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Metal-poor ultracool dwarfs in the Euclid era
    Metal-poor ultracool dwarfs (ultracool subdwarfs, including very-low-mass stars and brown dwarfs) are tracers of the pristine chemical composition at early phases in the assembly of the Milky Way. They are poorly understood because they are extremely faint and rare. Our aims are to improve the knowledge of ultracool subdwarf candidates, to break
    Zhang, Jun-Yan Jerry et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..703Z
    Número de citas
    0
  • Sin árbitro
    Close visual binaries among planetary-mass objects in star-forming regions: the HST view
    Over the past decade, microlensing surveys in field stars and the Gaia-informed census of nearby star-forming regions have convincingly demonsrated the presence of a significant population of free-floating planetary-mass objects. The origin of these objects is still debated, with the main plausible scenarios being: the dynamical ejection from a
    Duchene, Gaspard et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1613D
    Número de citas
    0
  • Sin árbitro
    Multi-epoch precise photometry from the ground: MUDEHaR, magnetic O stars and everything around
    MUDEHaR has completed its first of five years of project, and all the information is already available for exploitation. MUDEHaR is a multi-epoch photometric survey with two narrow filters in Hα and the calcium triplet window that uses T80Cam at the JAST80 telescope at Javalambre spanish astronomical observatory. It is obtaining ~50 epochs/year per
    Holgado, Gonzalo et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..124H
    Número de citas
    0