activity
20182026
most citedThe dispersal of protoplanetary discs. II: Photoevaporation models with observationally derived irradiating spectra

70 citations · 215 across the 21 of their papers we have counts for

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8 papers · 1 filter

astro-ph.SR2025★ 1 cited

The Radiowave Hunt for Young Stellar Object Emission and Demographics (RADIOHEAD): A Radio LuminositySpectral Type Dependence in TaurusAuriga YSOs

Ramisa Akther Rahman, Joshua Bennett Lovell, Eric W. Koch +4

We measure the radio continuum fluxes at the locations of all Gaiaconfirmed members of TaurusAuriga using Karl G. Jansky Very Large Array Sky Survey data (VLASS; 24…

astro-ph.SR2024

EWOCS-III: JWST observations of the supermassive star cluster Westerlund 1

M. G. Guarcello, V. Almendros-Abad, J. B. Lovell +29

The typically large distances, extinction, and crowding of Galactic supermassive star clusters have so far hampered the identification of their very low mass members, required to e…

astro-ph.SR2024

DECaPS and SMA discovery of a highly-inclined class I YSO with an outflow: IRAS 08235-4316

Joshua Bennett Lovell, Kristina Monsch, Garrett K. Keating +4

We present images of IRAS~08235--4316 with the Dark Energy Camera Plane Survey (DECaPS; spanning 0.398--1.034m, at resolution) and the Submillimeter Array (SMA; at…

astro-ph.SR2024

On Convective Turnover Times and Dynamos In Low-Mass Stars

Seth Gossage, Rocio Kiman, Kristina Monsch +7

The relationship between magnetic activity and Rossby number is one way through which stellar dynamos can be understood. Using measured rotation rates and X-ray to bolometric lumin…

astro-ph.SR2024★ 8 cited

High-resolution Pan-STARRS and SMA observations of IRAS 23077+6707: A giant edge-on protoplanetary disk

Kristina Monsch, Joshua B. Lovell, Ciprian T. Berghea +6

We present resolved images of IRAS 23077+6707 ("Dracula's Chivito") in 1.3 mm/225 GHz thermal dust and CO gas emission with the Submillimeter Array (SMA) and optical (0.5-$0.8\,μ\m…

astro-ph.SR2023

Linking circumstellar disk lifetimes to the rotational evolution of low-mass stars

Kristina Monsch, Jeremy J. Drake, Cecilia Garraffo +2

The high-energy radiation emitted by young stars can have a strong influence on their rotational evolution at later stages. This is because internal photoevaporation is one of the…

astro-ph.SR2023★ 3 cited

Three-dimensional, Time-dependent MHD Simulation of Disk-Magnetosphere-Stellar Wind Interaction in a T Tauri, Protoplanetary System

Ofer Cohen, Cecilia Garraffo, Jeremy Drake +4

We present a three-dimensional, time-dependent, MHD simulation of the short-term interaction between a protoplanetary disk and the stellar corona in a T Tauri system. The simulatio…

astro-ph.SR2019

White paper for Chandra cool attitude targets (CAT): Stellar activity with TESS and Chandra

Hans Moritz Günther, David A. Principe, Carl Melis +9

All cool stars show magnetic activity, and X-ray emission is the hallmark of this activity. Gaining an understanding of activity aids us in answering fundamental questions about st…