The Integral Field View of the Orion Nebula

This paper reviews the major advances achieved in the Orion Nebula through the use of integral field spectroscopy (IFS). Since the early work of Vasconcelos and collaborators in 2005, this technique has facilitated the investigation of global properties of the nebula and its morphology, providing ne...

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Main Author: Adal Mesa-Delgado
Format: Article
Language:English
Published: Wiley 2014-01-01
Series:Advances in Astronomy
Online Access:http://dx.doi.org/10.1155/2014/279320
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author Adal Mesa-Delgado
author_facet Adal Mesa-Delgado
author_sort Adal Mesa-Delgado
collection DOAJ
description This paper reviews the major advances achieved in the Orion Nebula through the use of integral field spectroscopy (IFS). Since the early work of Vasconcelos and collaborators in 2005, this technique has facilitated the investigation of global properties of the nebula and its morphology, providing new clues to better constrain its 3D structure. IFS has led to the discovery of shock-heated zones at the leading working surfaces of prominent Herbig-Haro objects as well as the first attempt to determine the chemical composition of Orion protoplanetary disks, also known as proplyds. The analysis of these morphologies using IFS has given us new insights into the abundance discrepancy problem, a long-standing and unresolved issue that casts doubt on the reliability of current methods used for the determination of metallicities in the universe from the analysis of H II regions. Results imply that high-density clumps and high-velocity flows may play an active role in the production of such discrepancies. Future investigations based on the large-scale IFS mosaic of Orion will be very valuable for exploring how the integrated effect of small-scale structures may have impact at larger scales in the framework of star-forming regions.
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spelling doaj-art-37293ea2e63e45a8bcdc38ef7fb38de82025-02-03T01:25:27ZengWileyAdvances in Astronomy1687-79691687-79772014-01-01201410.1155/2014/279320279320The Integral Field View of the Orion NebulaAdal Mesa-Delgado0Instituto de Astrofísica, Facultad de Física, Pontificia Universidad Católica de Chile, Avenida Vicuña Mackenna 4860, Macul, 782-0436, Santiago, ChileThis paper reviews the major advances achieved in the Orion Nebula through the use of integral field spectroscopy (IFS). Since the early work of Vasconcelos and collaborators in 2005, this technique has facilitated the investigation of global properties of the nebula and its morphology, providing new clues to better constrain its 3D structure. IFS has led to the discovery of shock-heated zones at the leading working surfaces of prominent Herbig-Haro objects as well as the first attempt to determine the chemical composition of Orion protoplanetary disks, also known as proplyds. The analysis of these morphologies using IFS has given us new insights into the abundance discrepancy problem, a long-standing and unresolved issue that casts doubt on the reliability of current methods used for the determination of metallicities in the universe from the analysis of H II regions. Results imply that high-density clumps and high-velocity flows may play an active role in the production of such discrepancies. Future investigations based on the large-scale IFS mosaic of Orion will be very valuable for exploring how the integrated effect of small-scale structures may have impact at larger scales in the framework of star-forming regions.http://dx.doi.org/10.1155/2014/279320
spellingShingle Adal Mesa-Delgado
The Integral Field View of the Orion Nebula
Advances in Astronomy
title The Integral Field View of the Orion Nebula
title_full The Integral Field View of the Orion Nebula
title_fullStr The Integral Field View of the Orion Nebula
title_full_unstemmed The Integral Field View of the Orion Nebula
title_short The Integral Field View of the Orion Nebula
title_sort integral field view of the orion nebula
url http://dx.doi.org/10.1155/2014/279320
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