36 citations · 115 across the 6 of their papers we have counts for
6 papers
Origin of the IRAS Vela Shell: New Insights from 3D Dust Mapping
Bore Annie Gao, Catherine Zucker, Tirupati Kumara Sridharan +15
The IRAS Vela Shell (IVS) is a structure of enhanced FIR emission located towards the Gum Nebula, a prominent region of emission in the local Milky Way shaped by various g…
Most nearby young star clusters formed in three massive complexes
Cameren Swiggum, João Alves, Robert Benjamin +9
Efforts to unveil the structure of the local interstellar medium and its recent star formation history have spanned the past seventy years. Recent studies utilizing precise data fr…
The Radcliffe Wave is Oscillating
Ralf Konietzka, Alyssa A. Goodman, Catherine Zucker +6
Our Sun lies within 300 pc of the 2.7-kpc-long sinusoidal chain of dense gas clouds known as the Radcliffe Wave. The structure's wave-like shape was discovered using 3D dust mappin…
VISIONS: The VISTA Star Formation Atlas -- I. Survey overview
Stefan Meingast, João Alves, Hervé Bouy +37
VISIONS is an ESO public survey of five nearby (d < 500 pc) star-forming molecular cloud complexes that are canonically associated with the constellations of Chamaeleon, Corona Aus…
Kinematics, Structure, and Mass Outflow Rates of Extreme Starburst Galactic Outflows
Serena Perrotta, Alison L. Coil, David S. N. Rupke +10
We present results on the properties of extreme gas outflows in massive (10), compact, starburst ($200 \, \rm M_{\odot} \ yr^{-1}…
Evidence of a vertical kinematic oscillation beyond the Radcliffe Wave
Lekshmi Thulasidharan, Elena D'Onghia, Eloisa Poggio +5
The Radcliffe Wave (RW) is a recently discovered sinusoidal vertical feature of dense gas in the proximity of the Sun. In the disk plane, it is aligned with the Local Arm. However,…