Bibcode
Rosado, M.; Rodríguez-González, A.; Velázquez, P. F.; Font, J.; Beckman, J. E.; Zaragoza-Cardiel, J.; Camps-Fariña, A.
Referencia bibliográfica
Monthly Notices of the Royal Astronomical Society, Volume 468, Issue 4, p.4134-4142
Fecha de publicación:
7
2017
Número de citas
5
Número de citas referidas
5
Descripción
Mass outflow generated by the dynamical feedback from massive stars is
currently a topic of great interest. Using a purpose-developed analysis
technique, and taking full advantage of the high kinematic and angular
resolution of our instrument, we have detected a number of expanding
superbubbles in the interacting pair of galaxies Arp 244 (NGC 4038/9),
commonly known as the Antennae. We used a Fabry-Pérot
interferometer GHαFaS to measure the profile of H α in
emission over the full extent of the object, except for the extended H i
tails. The superbubbles are found to be centred on most of the brightest
H ii regions, especially in the overlap area of the two merging
galaxies. We use measured sizes, expansion velocities and luminosities
of the shells to estimate most of the physical parameters of the
bubbles, including the kinetic energy of the expansion. In order to
assess the validity of our results and approximations, we perform a
hydrodynamic simulation and manage to reproduce well our best measured
superbubble with reasonable physical input assumptions. We also study
the sources of ionization of the shells, finding that at the current,
quite late stage of expansion, radiation from the remaining stars
dominates, although the effect of supernova shocks can still be
observed.
Proyectos relacionados
Estudios Cinemáticos, Estructurales y de Composición, de los Medios Interestelares e Intergalácticos
El objetivo básico del proyecto es investigar la evolución de las galaxias mediante el entendimiento de la interacción del medio interestelar y las estrellas. La técnica principal que utilizamos es la cinemática bidimensional de galaxias enteras observada por nuestro instrumento GHaFaS, un interferometro Fabry Perot en el telescopio William
Prof.
John E. Beckman