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20232026
most citedImpact of Resonance, Raman, and Thomson Scattering on Hydrogen Line Formation in Little Red Dots

14 citations · 39 across the 18 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.GA2025★ 1 cited

ODIN: A New Lyman Alpha Blob Selection Method, Sample, and Statistical Analysis at

Byeongha Moon, Yujin Yang, Kyoung-Soo Lee +26

Ly blobs (LABs) are large, spatially extended Ly-emitting objects whose nature remains unclear. Their statistical properties such as number densities and luminosity functions…

astro-ph.GA2025★ 14 cited

The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings

Alberto Torralba, Jorryt Matthee, Gabriele Pezzulli +22

The population of the Little Red Dots (LRDs) may represent a key phase of supermassive black hole (SMBH) growth. A cocoon of dense excited gas is emerging as key component to expla…

astro-ph.GA2025★ 1 cited

Lyman- Escape through Anisotropic Media

Silvia Almada Monter, Max Gronke, Seok-Jun Chang

The escape of Lyman- (Ly) radiation encodes valuable information on the neutral interstellar medium and is often used as a proxy for the escape of ionizing photons. Yet, the…

astro-ph.GA2025★ 14 cited

Impact of Resonance, Raman, and Thomson Scattering on Hydrogen Line Formation in Little Red Dots

Seok-Jun Chang, Max Gronke, Jorryt Matthee +1

Little Red Dots (LRDs) are compact sources at discovered through JWST spectroscopy. Their spectra exhibit broad Balmer emission lines (), alongside…

astro-ph.GA2025★ 2 cited

Ruling out dominant electron scattering in Little Red Dots' Rosetta Stone using multiple hydrogen lines

Matilde Brazzini, Francesco D'Eugenio, Roberto Maiolino +3

The majority of Little Red Dots (LRDs) hosting Active Galactic Nuclei (AGN) exhibits broad H emission, which recent studies propose originates from scattering off free electrons…

astro-ph.SR2025★ 3 cited

Evidence of a Disk-wind Origin for Fluorescent H in Classical T Tauri Stars

Matt Kalscheur, Kevin France, Brunella Nisini +8

We use FUV spectra of 36 T Tauri stars, predominately from 's ULLYSES program, to examine the kinematic properties of fluorescent H emission li…