The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
A new generation of wide-field emission-line surveys based on integral field units (IFU) is allowing us to obtain spatially resolved information of the gas-phase emission in nearby late-type galaxies, based on large samples of HII regions and full two-dimensional coverage. These observations are all...
Saved in:
Main Author: | Fernando Fabián Rosales-Ortega |
---|---|
Format: | Article |
Language: | English |
Published: |
Wiley
2013-01-01
|
Series: | Advances in Astronomy |
Online Access: | http://dx.doi.org/10.1155/2013/627867 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Multiepoch Observations of the Nearby Spiral Galaxy NGC 3938 with the Chandra X-Ray Observatory
by: Siddhi Raut, et al.
Published: (2025-01-01) -
Studying the Interstellar Medium of H II/BCD Galaxies Using IFU Spectroscopy
by: Patricio Lagos, et al.
Published: (2013-01-01) -
The Disk Wind Contribution to the Gamma-Ray Emission from the Nearby Seyfert Galaxy GRS 1734−292
by: Nobuyuki Sakai, et al.
Published: (2025-01-01) -
Analysis of ∼106 Spiral Galaxies from Four Telescopes Shows Large-Scale Patterns of Asymmetry in Galaxy Spin Directions
by: Lior Shamir
Published: (2022-01-01) -
Analysis of the Internal Radial Gradient of Chemical Abundances in Spiral Galaxies from CALIFA
by: A. F. S. Cardoso, et al.
Published: (2025-01-01)