Morphology and Kinematics of the High Excitation Planetary Nebula Hb 5

Bibcode
2000ASPC..199..397P
Pismis, Paris; Manteiga, Minia; Mampaso Recio, Antonio
Referencia bibliográfica

Asymmetrical Planetary Nebulae II: From Origins to Microstructures, ASP Conference Series, Vol. 199. Edited by J. H. Kastner, N. Soker, and S. Rappaport. ISBN: 1-58381-026-9, 2000, p. 397

Advertised on:
0
2000
Número de autores
3
Número de autores del IAC
1
Número de citas
6
Número de citas referidas
6
Descripción
The planetary nebula Hubble 5 represents a clear case of point- symmetry: a 180 deg rotation around its center would bring the object into fair coincidence. Long slit spectroscopy along different axis passing through the center of the nebula has been performed in order to map and analyse in detail the gas kinematics.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    European Solar Telescope expected performance
    The European Solar Telescope (EST) will be the biggest solar telescope in Europe and it is currently concluding its preliminary design that includes adaptive optics from its first light. In this phase of the project, the feasibility of the project is demonstrated and the design must meet the requirements after having mitigated the major risks. The
    Nuñez, Miguel et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1274N
    Número de citas
    0
  • Sin árbitro
    A multi-wavelength view of AGN feedback in the central kiloparsecs of quasar host galaxies
    Active galactic nuclei (AGN) winds and jets are potential drivers of multi-phase outflows and can significantly modify the interstellar medium (ISM) properties of their host galaxies. The Quasar Feedback (QSOFEED) project aims to investigate the impact of multi-phase quasar-driven outflows and jets on the nuclear regions of quasar host galaxies
    Audibert, Anelise et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1649A
    Número de citas
    0
  • Sin árbitro
    The Undiscovered Ultra Diffuse galaxies of the Local Group: predictions from constrained cosmological simulations
    Ultra-diffuse galaxies (UDGs) are attractive candidates to probe cosmological models and test theories of galaxy formation at low masses; however, they are difficult to detect because of their low surface brightness. In the Local Group a handful of UDGs have been found to date, most of which are satellites of the Milky Way and M31, and only two are
    Di Cintio, Arianna et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf..300D
    Número de citas
    0