XTE J1752-223: back to optical quiescence

Bibcode
2010ATel.2818....1C
Corral-Santana, J. M.; Rodríguez-Gil, P.; Guerra, J. C.; Casares, J.
Referencia bibliográfica

The Astronomer's Telegram, #2818

Fecha de publicación:
8
2010
Número de autores
4
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
2
Descripción
We observed the black hole candidate XTE J1752-223 (ATel #2258) with the William Herschel Telescope (WHT) and the ACAM imager/spectrograph at the Observatorio del Roque de los Muchachos, La Palma, Spain. 200-s exposures were taken in the R and I bands under photometric conditions and 0.6-0.7-arcsec seeing on Aug 24.887 and Aug 24.893, respectively. The object has dropped substantially since the optical re-brightening reported in ATel #2805.
Tipo
Sin árbitro
Agujeros negros

Te puede interesar

  • Sin árbitro
    Estimation of the hydrostatic-to-lensing mass bias from resolved cluster masses
    We present a study on the bias of hydrostatic masses with respect to lensing mass estimates for a sample of 53 clusters in a redshift range between z = 0.05 and 1.07. The M 500 mass for each cluster was inferred from X-ray and lensing data, without using a priori observable-mass scaling relations. Cluster masses of our reference analysis were
    Muñoz-Echeverría, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300033M
    Número de citas
    0
  • Sin árbitro
    IRAM 30-meter millimeter follow-up of deep OSIRIS-GTC optical surveys
    It is broadly accepted that CO is a reliable tracer of H2 in massive IR (L IR ≳ 10 9 L ⊙) galaxies, and that there are clear correlations between L IR and L' CO that are qualitatively independent of environment and even redshift. We present two tales on the search for 12CO emission from dusty star-forming galaxies in both field (Lockman Hole, z < 0
    Sánchez-Portal, M. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300047S
    Número de citas
    0
  • Sin árbitro
    The NIKA2 Sunyaev-Zeldovich Large Program. Sample and upcoming product public release
    The NIKA2 camera operating at the IRAM 30-m telescope excels in high-angular resolution mapping of the thermal Sunyaev-Zel'dovich effect towards galaxy clusters at intermediate and high-redshift. As part of the NIKA2 guaranteed-time, the SZ Large Program (LPSZ) aims at tSZ-mapping a representative sample of SZ-selected galaxy clusters in the
    Perotto, L. et al.

    Fecha de publicación:

    6
    2024
    Bibcode
    2024EPJWC.29300040P
    Número de citas
    0