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19982026
most citedA General Theory of Turbulence-Regulated Star Formation, From Spirals to ULIRGs

1.1k citations · 24.6k across the 330 of their papers we have counts for

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Showing astro-ph.SRShow all

37 papers · 1 filter

astro-ph.SR2022

Hyperion: The origin of the stars A far-UV space telescope for high-resolution spectroscopy over wide fields

Erika Hamden, David Schiminovich, Shouleh Nikzad +30

We present Hyperion, a mission concept recently proposed to the December 2021 NASA Medium Explorer announcement of opportunity. Hyperion explores the formation and destruction of m…

astro-ph.SR2022★ 5 cited

Theoretical and Observational Evidence for Coriolis Effects in Coronal Magnetic Fields Via Direct Current Driven Flaring Events

Darryl Z. Seligman, Leslie A. Rogers, Adina D. Feinstein +6

All stars produce explosive surface events such as flares and coronal mass ejections. These events are driven by the release of energy stored in coronal magnetic fields, generated…

astro-ph.SR2021★ 24 cited

Chronostar. II. Kinematic age and substructure of the Scorpius-Centaurus OB2 association

Maruša Žerjal, Michael J. Ireland, Timothy D. Crundall +2

The nearest region of massive star formation - the Scorpius-Centaurus OB2 association (Sco-Cen) - is a local laboratory ideally suited to the study of a wide range of astrophysical…

astro-ph.SR2020★ 59 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…

astro-ph.SR2019★ 5 cited

Dynamics of small grains in transitional discs

Mark R. Krumholz, Michael J. Ireland, Kaitlin M. Kratter

Transitional discs have central regions characterised by significant depletion of both dust and gas compared to younger, optically-thick discs. However, gas and dust are not deplet…

astro-ph.SR2019★ 17 cited

Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars

Arpita Roy, Ralph S Sutherland, Mark R Krumholz +2

The evolutionary paths taken by massive stars with remain substantially uncertain. They begin their lives as main sequence (MS) O-stars. Dependin…