activity
20212026
collaborators

6 papers

astro-ph.GA2026

The Multi-phase Biconical Outflow in the local IR-Luminous Merger IRASF01364-1042

Y. Song, V. U, J. Kader +37

We investigate the spatially-resolved ISM properties of the local (), IR-luminous (\,L), late-stage galaxy merger IRAS F01364-1042, comb…

astro-ph.GA2025

Warm and cold molecular gas in the cluster center of MACS 1931-26 with JWST and ALMA

L. Ghodsi, L. Kuhn, A. W. S. Man +9

We perform one of the first spatially resolved studies of warm (100 K) and cold (10-100 K) molecular gas in the circumgalactic medium (CGM), focusing on the brightest cluster ga…

astro-ph.GA2024

Molecular gas mass measurements of an active, starburst galaxy at using ALMA observations of the [CI], CO and dust emission

Hao-Tse Huang, Allison W. S. Man, Federico Lelli +7

We present new ALMA observations of a starburst galaxy at cosmic noon hosting a radio-loud active galactic nucleus: PKS 0529-549 at . To investigate the conditions of its c…

astro-ph.GA2024

Molecular gas excitation in the circumgalactic medium of MACS1931-26

L. Ghodsi, J. Zhou, P. Andreani +6

The evolution of galaxies is largely affected by exchanging material with their close environment, the circumgalactic medium (CGM). In this work, we investigate the CGM and the int…

astro-ph.GA2023

Star formation efficiency across large-scale galactic environments

Laya Ghodsi, Allison Man, Darko Donevski +4

Environmental effects on the evolution of galaxies have been one of the leading questions in galaxy studies for decades. In this work, we investigate the relationship between the s…

astro-ph.CO2021

Structure of cosmic web in non-linear regime: the nearest neighbour and spherical contact distributions

Mohammad Ansari Fard, Zahra Baghkhani, Laya Ghodsi +3

In non-linear scales, the matter density distribution is not Gaussian. Consequently, the widely used two-point correlation function is not adequate anymore to capture the matter de…