The chemical composition of the Orion star forming region: stars, gas and dust

Bibcode
2011BSRSL..80..255S
Simón-Díaz, S.; Nieva, M. F.; Przybilla, N.; Stasińska, G.
Referencia bibliográfica

Société Royale des Sciences de Liège, Bulletin, vol. 80, p. 255-259 (Proceedings of the 39th Liège Astrophysical Colloquium, held in Liège 12-16 July 2010, edited by G. Rauw, M. De Becker, Y. Nazé, J.-M. Vreux, P. Williams)

Fecha de publicación:
1
2011
Número de autores
4
Número de autores del IAC
0
Número de citas
3
Número de citas referidas
3
Descripción
We present a summary of main results from the studies performed in the series of papers The chemical composition of the Orion star forming region. We reinvestigate the chemical composition of B-type stars in the Orion OB1 association by means of state-of-the-art stellar atmosphere codes, atomic models and techniques, and compare the resulting abundances with those obtained from the emission line spectra of the Orion nebula (M42), and recent determinations of the Solar chemical composition.
Tipo
Sin árbitro

Te puede interesar

  • Sin árbitro
    Study of basaltic asteroids through their phase curves
    Introduction Classified as type-V, the basaltic asteroids of the Main Belt (MB), for the most part, are connected to Vesta's dynamic family. However, since the discovery of the V-type asteroid (1459) Magnya in the outer MB, several new asteroids have been found in different regions, including V-types from inner regions not belonging to the Vesta
    Arcoverde, Plicida et al.

    Fecha de publicación:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Número de citas
    0
  • 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