activity
20192024
most citedSolar oxygen abundance

94 citations · 145 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024

Excitation mechanisms of C II optical permitted lines in ionized nebulae

E. Reyes-Rodríguez, J. E. Méndez-Delgado, J. García-Rojas +4

Context. Carbon is the fourth most abundant element in the universe and its distribution is critical to understanding stellar evolution and nucleosynthesis. In optical studies of i…

astro-ph.SR2024

Constraining Protoplanetary Disk Winds from Forbidden Line Profiles with Simulation-based Inference

Ahmad Nemer, ChangHoon Hahn, Jiaxuan Li +2

Protoplanetary disks are the sites of vigorous hydrodynamic processes, such as accretion and outflows, and ultimately establish the conditions for the formation of planets. The pro…

astro-ph.EP2024★ 2 cited

Photoevaporation from Inner Protoplanetary Disks Confronted with Observations

Yiren Lin, Lile Wang, Min Fang +2

The decades-long explorations on the dispersal of protoplanetary disks involve many debates about photoevaporation versus magnetized wind launching mechanisms. This letter argues t…

astro-ph.SR2023

Line profiles of forbidden emission lines and what they can tell us about protoplanetary disk winds

Ahmad Nemer, Jeremy Goodman

Emission in forbidden lines of oxygen, neon, and other species are commonly used to trace winds from protoplanetary disks. Using Cloudy, we calculate such emission for parametrized…

astro-ph.SR2023★ 27 cited

High-resolution [O I] line spectral mapping of TW Hya supportive of a magnetothermal wind

Min Fang, Lile Wang, Gregory J. Herczeg +6

Disk winds are thought to play a critical role in the evolution and dispersal of protoplanetary disks. A primary diagnostic of this physics is emission from the wind, especially in…

astro-ph.SR2021★ 94 cited

Solar oxygen abundance

Maria Bergemann, Richard Hoppe, Ekaterina Semenova +10

Motivated by the controversy over the surface metallicity of the Sun, we present a re-analysis of the solar photospheric oxygen (O) abundance. New atomic models of O and Ni are use…

astro-ph.SR2020★ 12 cited

The role of FUV Pumping in exciting the [Oi] lines in Protostellar Disks and Winds

Ahmad Nemer, Jeremy Goodman, Lile Wang

We use Cloudy to re-examine excitation of [Oi] 6300 A and [Oi] 5577 A in the X-ray driven photo-evaporative wind models of Owen and collaborators, and in more recent magnetothermal…

astro-ph.SR2019★ 10 cited

First evidence of enhanced recombination in astrophysical environments and the implications for plasma diagnostics

A. Nemer, N. C. Sterling, J. Raymond +6

We report the first unambiguous observational evidence of Rydberg Enhanced Recombination (RER), a potentially important recombination mechanism that has hitherto been unexplored in…