activity
20012026
most citedConsistent dust and gas models for protoplanetary disks. I. Disk shape, dust settling, opacities, and PAHs

379 citations · 1.8k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.EP2026

Molecular diagnostics for the mid-infrared emission of planet-forming disks. Carbon and oxygen elemental abundances

Aditya M. Arabhavi, Inga Kamp, Ewine F. van Dishoeck +8

Mid-infrared observations of planet-forming disks reveal a wide diversity in molecular spectra. Carbon and oxygen abundances play a central role in setting the chemical environment…

gr-qc2025

SMBH shadows: gravity fingerprints revealed by spectral line background radiation

Konstantinos Kostaros, Padelis Papadopoulos, Wing-Fai Thi +1

SMBHs at the centers of galaxies, illuminated by their accretion disks, can reveal valuable information on BH spacetimes via their shadows, which can be used for strong-gravity tes…

gr-qc2025

Einstein ring fingerprint around supermassive black holes illuminated by broad line region spectral lines

Konstantinos Kostaros, George Pappas, Padelis Papadopoulos +1

The continuum emission from the hot and ionized inner regions of accretion disks around supermassive black holes (SMBHs), which is strongly lensed by the light ring (i.e., the unst…

astro-ph.GA2024

The neutral gas phase nearest to supermassive black holes

Wing-Fai Thi, Padelis Papadopoulos

Broad Line Regions (BLRs) are known to contain gravitationally-bound gas within r~(few) 10^2-10^3 Schwarszchild radii (Rs) near supermassive black holes (SMBHs) in Active Galactic…

astro-ph.GA2023★ 6 cited

First observations of warm and cold methanol in Class 0/I proto-brown dwarfs

B. Riaz, W. -F. Thi, M. N. Machida

We present results from the first molecular line survey to search for the fundamental complex organic molecule, methanol (CHOH), in 14 Class 0/I proto-brown dwarfs (proto-BDs…

astro-ph.GA2023★ 8 cited

Simulation of CHOH ice UV photolysis under laboratory conditions

W. R. M. Rocha, P. Woitke, S. Pilling +5

Methanol is the most complex molecule securely identified in interstellar ices and is a key chemical species for understanding chemical complexity in astrophysical environments. Im…