Integral Field Spectroscopy of Planetary Nebulae with MUSE

Bibcode
2020Galax...8...31W
DOI
10.3390/galaxies8020031
Walsh, Jeremy R.; Monreal-Ibero, Ana
Referencia bibliográfica

Galaxies

Fecha de publicación:
4
2020
Número de autores
2
Número de autores del IAC
1
Número de citas
7
Número de citas referidas
7
Descripción
The Multi-Unit Spectroscopic Explorer (MUSE) is a large integral field unit mounted on the ESO Very Large Telescope. Its spatial (60 arcsecond field) and wavelength (4800-9300Å) coverage is well suited to detailed imaging spectroscopy of extended planetary nebulae, such as in the Galaxy. An overview of the capabilities of MUSE applied to Planetary Nebulae (PNe) is provided together with the specific advantages and disadvantages. Some examples of archival MUSE observations of PNe are provided. MUSE datacubes for two targets (NGC 3132 and NGC 7009) are analyzed in detail, and they are used to show the advances achievable for planetary nebula studies. Prospects for further MUSE observations of PNe and a broader analysis of existing datasets are outlined.
Proyectos relacionados
Los agujeros negros supermasivos modifican la distribución de gas molecular en la región central de las galaxias. Crédito: HST y C. Ramos Almeida.
Actividad Nuclear en Galaxias: una Perspectiva 3D del Núcleo y su Entorno

Nuestro proyecto puede dividirse en dos líneas principales de investigación. En primer lugar, el estudio de los vientos producidos por cuásares luminosos oscurecidos y del impacto que estos tienen en sus galaxias anfitrionas (retroalimentación del AGN). Para ello hemos obtenido observaciones infrarrojas y ópticas con los instrumentos del Gran

Cristina
Ramos Almeida
En ejecución
Tipo
Con árbitro
Formación y Evolución de Galaxias (FYEG)
Instrumentación infrarroja
Instrumentación visible

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