Hα Emission from High‐Velocity Clouds and Their Distances
The Astrophysical Journal2003Vol. 597(2), pp. 948–956
Citations Over TimeTop 10% of 2003 papers
Abstract
We present deep Ha spectroscopy toward several high-velocity clouds (HVCs), which vary in structure from compact HVCs (CHVCs) to the Magellanic Stream. The clouds range from being bright (∼640 mR) to having upper limits on the order of 30-70 mR. The Hα
Related Papers
- → Equilibrium models of the Milky Way mass are biased high by the LMC(2020)67 cited
- → The Local Group Mass in the Light of Gaia(2022)36 cited
- → Predictions of distance within the Local Group(1985)18 cited
- → On the Motion in the Local Group of Galaxies(2007)
- → The LMC Intermediate and Old Populations(1999)