Formation, Evolution and Disruption of Giant HII regions.

Bibcode
1996imsf.proc..573M
Muñoz-Tuñon, C.; Tenorio-Tagle, G.; Castaneda, H. O.; Terlevich, R.
Bibliographical reference

The interplay between massive star formation, the ISM and galaxy evolution. Proceedings of the 11th IAP Astrophysics meeting. edited by D. Kunth, B. Guiderdoni, M. Heydari-Malayeri, T. X. Thuan. Editions Frontieres, page 573

Advertised on:
0
1996
Number of authors
4
IAC number of authors
0
Citations
0
Refereed citations
0
Description
The distribution of velocity dispersion versus intensity, corresponding to the emission of the ionized gas over a giant HII region is explained within the framework of the cometary stirring model. The development of shells and loops generated by massive stars, which finally cause the cloud disruption, can also be followed with this representation.
Type
Non-refereed

It may interest you

  • Non-refereed
    Evaluating hydrodynamical simulations of galaxy formation with a variance analysis of optical spectra
    Cosmological hydrodynamical simulations, such as EAGLE and IllustrisTNG, provide valuable insights when coupled with high-quality survey data, enhancing our comprehension of galaxy evolution. In this work, we adopt a variance analysis of subsets of continuum-subtracted Sloan Digital Sky Survey (SDSS) spectra by Sharbaf+2023 and evaluate equivalent
    Sharbaf, Zahra et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1174S
    Citations
    0
  • Non-refereed
    From metal-poor to metal-rich: new insights on Milky Way bar, bulge and disc with machine learning and Gaia.
    Machine Learning applications such as the hybrid-CNN (Guigluon et al. 2024) allows to homogeneously combine Gaia RVS spectra, photometry (G, BP, RP), parallaxes and the XP coefficients to obtain precise stellar parameters down to S/N=15. In this contribution, I will focus on the scientific applications and new results facilitated by this machine
    Nepal, Samir et al.

    Advertised on:

    7
    2024
    Bibcode
    2024eas..conf.1623N
    Citations
    0
  • Non-refereed
    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
    Citations
    0