activity
20242026
most citedComparing extragalactic megahertz-peaked spectrum and gigahertz-peaked spectrum sources

9 citations · 9 across the 3 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2026

Up in smoke: carbon-destruction in the terrestrial planet-forming region of a young Class I disk

F. J. Ballieux, M. K. McClure, E. A. Bergin +5

Earth's surface and deep mantle are strongly depleted in carbon compared to the Sun. Sublimation of solid carbonaceous material in the inner midplanes of young disks could cause th…

astro-ph.SR2026

A breath of fresh air: Oxygen enhancement from silicate sublimation during early protostellar evolution

F. J. Ballieux, M. K. McClure, Ł. Tychoniec +6

Recently, an analog to the t = 0 moment of our Solar System's meteoritic record was identified for the first time around the Class I protostar HOPS-315. Crystalline silicates were…

astro-ph.GA2025

The evolution of extragalactic peaked-spectrum sources down to 54 megahertz

Sai Zhai, Anniek J. Gloudemans, Gülay Gürkan +4

Peaked-spectrum (PS) sources, known for their distinct peaked radio spectra, represent a type of radio-loud active galactic nuclei (AGN). Among these, megahertz-peaked spectrum (MP…

astro-ph.GA2024★ 9 cited

Comparing extragalactic megahertz-peaked spectrum and gigahertz-peaked spectrum sources

F. J. Ballieux, J. R. Callingham, H. J. A. Röttgering +1

Recent sensitive wide-field radio surveys, such as the LOFAR Two Meter Sky Survey (LoTSS), the LOFAR LBA Sky Survey (LoLSS), and the Very Large Array Sky Survey (VLASS), enable the…

astro-ph.GA2024

At the end of cosmic noon: Short gas depletion times in unobscured quasars at 1

M. Frias Castillo, M. Rybak, J. Hodge +8

Unobscured quasars (QSOs) are predicted to be the final stage in the evolutionary sequence from gas-rich mergers to gas-depleted, quenched galaxies. Studies of this population, how…