activity
19972023
most citedStructural Analysis of Molecular Clouds: Dendrograms

580 citations · 9.7k across the 129 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2023★ 98 cited

The star formation history of the Sco-Cen association. Coherent star formation patterns in space and time

Sebastian Ratzenböck, Josefa E. Großschedl, João Alves +13

We reconstruct the star formation history of the Sco-Cen OB association using a novel high-resolution age map of the region. We develop an approach to produce robust ages for Sco-C…

astro-ph.SR2021★ 34 cited

The Oph region revisited with Gaia EDR3

Natalie Grasser, Sebastian Ratzenböck, João Alves +10

Context. Young and embedded stellar populations are important probes of the star formation process. Paradoxically, we have a better census of nearby embedded young populations than…

astro-ph.SR2016★ 15 cited

The first stars of the Rho Ophiuchi Dark Cloud. XMM-Newton view of Rho Oph and its neighbors

Ignazio Pillitteri, Scott J. Wolk, Hope H. Chen +1

Star formation in molecular clouds can be triggered by the dynamical action of winds from massive stars. Furthermore, X-ray and UV fluxes from massive stars can influence the life…

astro-ph.SR2016★ 85 cited

Misalignment of Outflow Axes in the Proto-Multiple Systems in Perseus

Katherine I. Lee, Michael M. Dunham, Philip C. Myers +9

We investigate the alignment between outflow axes in nine of the youngest binary/multiple systems in the Perseus Molecular Cloud. These systems have typical member spacing larger t…

astro-ph.SR2014★ 6 cited

Smooth X-ray variability from Ophiuchi A+B. A strongly magnetized primary B2 star?

Ignazio Pillitteri, Scott J. Wolk, Alyssa Goodman +1

X-rays from massive stars are ubiquitous yet not clearly understood. In an XMM-Newton observation devoted to observe the first site of star formation in the Ophiuchi dark cloud…

astro-ph.SR2011★ 31 cited

Observing Turbulent Fragmentation in Simulations: Predictions for CARMA and ALMA

Stella S. R. Offner, John Capodilupo, Scott Schnee +1

Determining the initial stellar multiplicity is a challenging problem since protostars are faint and deeply embedded at early times; once formed, multiple protostellar systems may…