CI Cam: Observations of the Dust Envelope Diameter

Bibcode
1998AAS...193.5206T
Traub, W. A.; Millan-Gabet, R. S.; Garcia, M. R.
Referencia bibliográfica

American Astronomical Society, 193rd AAS Meeting, #52.06; Bulletin of the American Astronomical Society, Vol. 30, p.1330

Fecha de publicación:
12
1998
Número de autores
3
Número de autores del IAC
0
Número de citas
2
Número de citas referidas
2
Descripción
We spatially resolved the symbiotic star CI Cam, about 6 months after its April 1998 outburst, using the IOTA stellar interferometer. We measured the diameter of the dust shell in the H and K infrared bands over a range of position angles. We will discuss the relationship between these results and other ongoing observations of CI Cam.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    The LiteBIRD mission to explore cosmic inflation
    LiteBIRD, the next-generation cosmic microwave background (CMB) experiment, aims for a launch in Japan's fiscal year 2032, marking a major advancement in the exploration of primordial cosmology and fundamental physics. Orbiting the Sun-Earth Lagrangian point L2, this JAXA-led strategic L-class mission will conduct a comprehensive mapping of the CMB
    Ghigna, T. et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13092E..28G
    Número de citas
    0
  • Sin árbitro
    Performance of MAGIC stellar intensity interferometer and expansion to MAGIC + CTAO-LST1 stellar intensity interferometer
    A new generation of optical intensity interferometers are emerging in recent years taking advantage of the existing infrastructure of Imaging Atmospheric Cherenkov Telescopes (IACTs). The MAGIC SII (Stellar Intensity Interferometer) in La Palma, Spain, has been operating since its first successful measurements in 2019 and its current design allows
    Cifuentes, Alejo et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13095E..27C
    Número de citas
    0
  • Sin árbitro
    GTC adaptive optics integration in telescope and first commissioning results
    The Adaptive Optics (AO) of the Gran Telescopio Canarias (GTC) is a single conjugate postfocal system, integrated in one of the Nasmyth platforms of the telescope. GTC is located in the Observatory of Roque de Los Muchachos (ORM) in the island of La Palma, Spain. GTCAO is based on a single deformable mirror (DM) with 373 actuators, conjugated to
    Reyes García-Talavera, Marcos et al.

    Fecha de publicación:

    8
    2024
    Bibcode
    2024SPIE13097E..0ER
    Número de citas
    0