Integral Field Spectroscopy of Planetary Nebulae with MUSE

Integral Field Spectroscopy of Planetary Nebulae with MUSE

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...

Deskribapen osoa

Xehetasun bibliografikoak
Egile Nagusiak:	Jeremy R. Walsh, Ana Monreal-Ibero
Formatua:	Artikulua
Hizkuntza:	English
Argitaratua:	MDPI AG 2020-04-01
Saila:	Galaxies
Gaiak:	optical spectroscopy integral field spectroscopy planetary nebulae emission lines physical conditions abundances
Sarrera elektronikoa:	https://www.mdpi.com/2075-4434/8/2/31

Antzeko izenburuak

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THE MASSES OF THE IONIZED GAS OF PLANETARY NEBULAE ENVELOPES IN LARGE MAGELLANIC CLOUD
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Toward Precision Cosmology with Improved Planetary Nebula Luminosity Function Distances Using VLT-MUSE. II. A Test Sample from Archival Data
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A Preferred Orientation Angle for Bipolar Planetary Nebulae
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ALMA Detection of Masers and Dasars in the Hydrogen Recombination Lines of the Planetary Nebula Mz3
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Millimetre Observations of Maser-Emitting Planetary Nebulae
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