most citedThe Timescales of Embedded Star Formation as Observed in STARFORGE

5 citations · 5 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2026

Dust-Embedded Star Formation: Bridging Magellanic Cloud Studies of Massive Young Stellar Objects to Nearby Spiral Galaxies

M. Jimena Rodríguez, Rémy Indebetouw, Janice C. Lee +13

We use JWST NIRCam and MIRI imaging at 2, 4, 10, and 21 um to study young, dusty compact sources in four nearby galaxies at distances of ~ 1-5Mpc (M33, NGC300, NGC7793, and NGC5068…

astro-ph.SR2026

Introducing PxP: A Population Synthesis Framework for Predicting YSO Properties

J. Peltonen, E. Rosolowsky, A Ginsburg +3

The most direct method of measuring the star formation rate is with young stellar objects (YSOs), but this requires high-resolution observations and high-quality models. Using the…

astro-ph.GA2026

Comparing the Relation inside a Giant Molecular Cloud

Carlos G. Román-Zúñiga, Aina Palau, Javier Ballesteros-Paredes +3

In this paper we present a simple analysis around scaling relations derived from the Schmidt conjecture for star-forming molecular clouds, at the intra-cloud scale. Using a hierarc…

astro-ph.SR20265 cited

The Timescales of Embedded Star Formation as Observed in STARFORGE

Tobin M. Wainer, Julianne J. Dalcanton, Michael Y. Grudić +7

Star formation occurs within dusty molecular clouds that are then disrupted by stellar feedback. However, the timing and physical mechanisms that govern the transition from deeply…

astro-ph.GA2025

A First-look at Spatially-resolved Infrared Supernova Remnants in M33 with JWST

Sumit K. Sarbadhicary, Erik Rosolowsky, Adam K. Leroy +12

We present the first spatially-resolved infrared images of supernova remnants (SNRs) in M33 with the unprecedented sensitivity and resolution of JWST. We analyze 40 SNRs in four JW…

astro-ph.SR2025

A framework for modeling the evolution of young stellar objects

Theo Richardson, Adam Ginsburg, Erik Rosolowsky +2

Measuring properties of young stellar objects (YSOs) is necessary for probing the pre-main-sequence evolution of stars. As YSOs exhibit complex geometry, measurement generally enta…