output
20112026
most citedOn Instrumental Variables Estimation of Causal Odds Ratios

117 citations

Showing astro-ph.GAShow all

26 papers · 1 filter

astro-ph.GA2024★ 5 cited

Assessing the accuracy of the star formation rate measurements by direct star count in molecular clouds

Sami Dib, Jian Wen Zhou, Sébastien Comerón +8

Star formation estimates based on the counting of YSOs is commonly applied to nearby star-forming regions in the Galaxy. With this method, the SFRs are measured using the counts of…

astro-ph.GA2020★ 26 cited

The structure and characteristic scales of molecular clouds

Sami Dib, Sylvain Bontemps, Nicola Schneider +8

The structure of molecular clouds (MCs) holds important clues on the physical processes that lead to their formation and subsequent evolution. While it is well established that tur…

astro-ph.GA2019★ 5 cited

Time-dependent evolution of the protoplanetary discs with magnetic winds

Mohsen Shadmehri, Sayyedeh Masoumeh Ghoreyshi

We study the evolution of the protoplanetary discs (PPDs) in the presence of magnetically driven winds with the stress relations motivated by the non-ideal MHD disc simulations. Co…

astro-ph.GA2019★ 1 cited

Linear Analysis of the Nonaxisymmetric Secular Gravitational Instability

Mohsen Shadmehri, Razieh Oudi, Gohar Rastegarzadeh

In protoplanetary discs (PPDs) consisting of gas and dust particles, fluid instabilities induced by the drag force, including secular gravitational instability (SGI) can facilitate…

astro-ph.GA2018★ 3 cited

Properties of an accretion disc with a power-law stress-pressure relationship

Mohsen Shadmehri, Fazeleh Khajenabi, Sami Dib +1

Recent numerical simulations of magnetized accretion discs show that the radial-azimuthal component of the stress tensor due to the magnetorotational instability (MRI) is well repr…

astro-ph.GA2018★ 7 cited

Evolution of circumbinary protoplanetary disks with photoevaporative winds driven by External Far Ultraviolet Radiation

Mohsen Shadmehri, S. M. Ghoreyshi, N. Alipour

Lifetimes of protoplanetary disks (PPDs) are believed to be severely constrained by material depleting mechanisms, including photoevaporative winds due to the host star radiation o…