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
    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.

    Advertised on:

    9
    2024
    Bibcode
    2024EPSC...17..999A
    Citations
    0
  • Non-refereed
    Conceptual design of the infrared integral field spectropolarimeter for the European Solar Telescope
    The European Solar Telescope (EST) will be Europe's most ambitious ground-based infrastructure in solar physics. It will have a primary mirror with a diameter of 4.2m, which will make it the largest in Europe, and of identical aperture as the largest solar telescope available worldwide, namely the Daniel K. Inouye Telescope (DKIST) installed at the
    Quintero Noda, C. et al.

    Advertised on:

    8
    2024
    Bibcode
    2024SPIE13094E..2CQ
    Citations
    0
  • Non-refereed
    Detector upgrade in EMIR@GTC: on-sky performances
    EMIR was shipped to the GTC on May 2016 and had its first light on June 2016. Since the beginning, the EMIR performances have been severely hampered by the many instabilities in the infrared detector, a 2048x2048 Hawaii2, built with the old original technology of the Teledyne Hawaii series. Despite of this, the instrument has proven to be powerful
    Garzón, Francisco et al.

    Advertised on:

    7
    2024
    Bibcode
    2024SPIE13096E..27G
    Citations
    0