Bibcode
Núñez-Díaz, M.; Mesa-Delgado, A.; Esteban, C.; López-Martín, L.; García-Rojas, J.; Luridiana, V.
Bibliographical reference
Monthly Notices of the Royal Astronomical Society, Volume 421, Issue 4, pp. 3399-3408.
Advertised on:
4
2012
Citations
10
Refereed citations
9
Description
We present results from integral field optical spectroscopy with the
Potsdam Multi-Aperture Spectrograph of the Herbig-Haro (HH) object HH
204, with a spatial sampling of 1 × 1 arcsec2. We have
obtained maps of different emission lines, physical conditions and ionic
abundances from collisionally excited lines. The ionization structure of
the object indicates that the head of the bow shock is optically thick
and has developed a trapped ionization front. The density at the head is
at least five times larger than in the background ionized gas. We
discover a narrow arc of high Te([N II]) values delineating
the southeast edge of the head. The temperature in this zone is about
1000 K higher than in the rest of the field and should correspond to a
shock-heated zone at the leading working surface of the gas flow. This
is the first time this kind of feature is observed in a photoionized HH
object. We find that the O+ and O abundance maps show
anomalous values at separate areas of the bow shock probably due to: (a)
overestimation of the collisional de-excitation effects of the [O II]
lines in the compressed gas at the head of the bow shock, and (b) the
use of a too high Te([N II]) at the area of the leading
working surface of the flow.
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Physics of Ionized Nebulae
The research that is being carried out by the group can be condensed into two main lines: 1) Study of the structure, dynamics, physical conditions and chemical evolution of Galactic and extragalactic ionized nebulae through detailed analysis and modelization of their spectra. Investigation of chemical composition gradients along the disk of our
Jorge
García Rojas