activity
20052009
most citedLarge Scale Flows from Orion-South

35 citations · 87 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.GA20091 cited

What can we learn about the kinematics of bright extragalactic planetary nebulae

M. G. Richer, S. -H. Baez, J. A. Lopez +2

We present high resolution spectroscopy in the [\ion{O}{3}]5007 and H lines of bright planetary nebulae in the Milky Way bulge and the dwarf galaxies M32, Fornax, Sagittarius…

astro-ph200827 cited

The Acceleration of the Nebular Shells in Planetary Nebulae in the Milky Way Bulge

Michael G. Richer, Jose Alberto Lopez, Margarita Pereyra +3

We present a systematic study of line widths in the [\ion{O}{3}]5007 and H lines for a sample of 86 planetary nebulae in the Milky Way bulge based upon spectroscopy obtained…

astro-ph200824 cited

The planetary nebula NGC 1360, a test case of magnetic collimation and evolution after the fast wind

M. T. Garcia-Diaz, J. A. López, G. Garcia-Segura +2

The central star of this nebula has an observed intense magnetic field and the fast wind is no longer present, indicating that a back flow process has probably developed. Long-slit…

astro-ph200735 cited

Large Scale Flows from Orion-South

W. J. Henney, C. R. O'Dell, Luis A. Zapata +3

Multiple optical outflows are known to exist in the vicinity of the active star formation region called Orion-South (Orion-S). We have mapped the velocity of low ionization feature…

astro-ph2005

Photoevaporation Flows in Blister HII Regions: I. Smooth Ionization Fronts and Application to the Orion Nebula

W. J. Henney, S. J. Arthur, Ma. T. Garcia-Diaz

We present hydrodynamical simulations of the photoevaporation of a cloud with large-scale density gradients, giving rise to an ionized, photoevaporation flow. The flow is found to…