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dc.date.accessioned 2024-06-25T17:56:18Z
dc.date.available 2024-06-25T17:56:18Z
dc.date.issued 2019
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/167505
dc.description.abstract Star formation processes can be found in colliding galaxies, where the gas compression can trigger the formation of giant star-forming regions. We present the results from a detailed kinematic analysis in a sample of HII regions located in three strongly interacting galaxies. The velocity dispersion and the luminosity of the multiple-components analyzed in the emission-line profiles suggest that these star-forming objects correspond to giant complexes. In addition, the star formation rates and the ionization state in these regions revealed the presence of ongoing star formation events. en
dc.format.extent 125-130 es
dc.language es es
dc.subject galaxies: kinematics es
dc.subject star formation es
dc.subject ISM es
dc.title The internal kinematic of star-forming regions in interacting galaxies en
dc.type Objeto de conferencia es
sedici.identifier.isbn 978-987-24948-6-5 es
sedici.creator.person Firpo, Verónica es
sedici.creator.person Muthukrishna, Daniel es
sedici.creator.person Campuzano Castro, Federico es
sedici.creator.person Bosch, Guillermo Luis es
sedici.creator.person Hägele, Guillermo Federico es
sedici.creator.person Torres Flores, Sergio es
sedici.creator.person Cardaci, Mónica Viviana es
sedici.subject.materias Ciencias Astronómicas es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Astrofísica de La Plata es
sedici.subtype Objeto de conferencia es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.date.exposure 2019-03
sedici.relation.event II Workshop on Chemical Abundances in Gaseous Nebulae: Open problems in Nebular Astrophysics (Brasil, 11 al 14 de marzo de 2019) es
sedici.description.peerReview peer-review es
sedici.relation.bookTitle Chemical abundances in gaseous nebulae: open problems in nebular astrophysics es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Excepto donde se diga explícitamente, este item se publica bajo la siguiente licencia Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)