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...
Κύριοι συγγραφείς: | Jeremy R. Walsh, Ana Monreal-Ibero |
---|---|
Μορφή: | Άρθρο |
Γλώσσα: | English |
Έκδοση: |
MDPI AG
2020-04-01
|
Σειρά: | Galaxies |
Θέματα: | |
Διαθέσιμο Online: | https://www.mdpi.com/2075-4434/8/2/31 |
Παρόμοια τεκμήρια
-
Studying Nearby Galactic Planetary Nebulae with MUSE: On the Physical Properties of IC 418
ανά: Ana Monreal-Ibero , κ.ά.
Έκδοση: (2022-01-01) -
SATELLITE: Application to Planetary Nebulae IFU Data
ανά: Stavros Akras, κ.ά.
Έκδοση: (2022-02-01) -
Spectroscopy of Planetary Nebulae with Herschel: A Beginners Guide
ανά: Katrina Exter
Έκδοση: (2018-07-01) -
Optical Spectroscopy and Photoionization Model of Planetary Nebula NGC 6572
ανά: Muhammad Fajrin, κ.ά.
Έκδοση: (2024-01-01) -
Whither or Wither the Sulfur Anomaly in Planetary Nebulae?
ανά: Shuyu Tan, κ.ά.
Έκδοση: (2024-01-01)