activity
20182021
most citedFormation and Evolution of Disks around Young Stellar Objects

74 citations · 223 across the 5 of their papers we have counts for

collaborators

11 papers

astro-ph.HE20221 cited

A Multiwavelength Study of the Massive Colliding Wind Binary WR 20a: A Possible Progenitor for Fast-Spinning LIGO Binary Black Hole Mergers

Grace M. Olivier, Laura A. Lopez, Katie Auchettl +7

WR 20a is the most massive close-in binary known in our Galaxy. It is composed of two 80 M Wolf-Rayet stars with a short period of 3.7 days in the open cl…

astro-ph.GA202231 cited

Effects of the environment on the multiplicity properties of stars in the STARFORGE simulations

Dávid Guszejnov, Aman N. Raju, Stella S. R. Offner +4

Most observed stars are part of a multiple star system, but the formation of such systems and the role of environment and various physical processes is still poorly understood. We…

astro-ph.SR20216 cited

Blowing Bubbles around Intermediate-Mass Stars: Feedback from Main-Sequence Winds is not Enough

Anna L. Rosen, Stella S. R. Offner, Michael M. Foley +1

Numerous spherical ``shells" have been observed in young star-forming environments that host low- and intermediate-mass stars. These observations suggest that these shells may be p…

astro-ph.GA202021 cited

Continuity of accretion from clumps to Class 0 high-mass protostars in SDC335

A. Avison, G. A. Fuller, N. Peretto +6

The IRDC SDC335.579-0.292 (SDC335) is a massive star-forming cloud found to be globally collapsing towards one of the most massive star forming cores in the Galaxy. SDC335 hosts th…

astro-ph.GA2020

Evolution of Stellar Feedback in HII Regions

Grace M. Olivier, Laura A. Lopez, Anna L. Rosen +4

Stellar feedback is needed to produce realistic giant molecular clouds (GMCs) and galaxies in simulations, but due to limited numerical resolution, feedback must be implemented usi…

astro-ph.SR202059 cited

The Role of Outflows, Radiation Pressure, and Magnetic Fields in Massive Star Formation

Anna L. Rosen, Mark R. Krumholz

Stellar feedback in the form of radiation pressure and magnetically-driven collimated outflows may limit the maximum mass that a star can achieve and affect the star-formation effi…