collaborators

6 papers

astro-ph.EP2025

Hubble reveals complex multi-scale structure in the edge-on protoplanetary disk IRAS 23077+6707

Kristina Monsch, Joshua B. Lovell, Karl R. Stapelfeldt +11

We present high-resolution () Hubble Space Telescope (HST)/Wide Field Camera 3 (WFC3) imaging of the near edge-on () protoplanetary disk IRAS 23077…

astro-ph.EP2025

SMA and NOEMA reveal asymmetric sub-structure in the protoplanetary disk of IRAS23077+6707

Joshua B. Lovell, Leon Trapman, Kristina Monsch +5

We present high-resolution data of IRAS 23077+6707 (`Dracula's Chivito') with the Submillimeter Array (SMA at 1.33 mm/225.5 GHz) and the Northern Extended Millimeter Array (NOEMA a…

astro-ph.SR2025

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

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; a…

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

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\…