Non-isothermal filaments in equilibrium
S. Recchi (1), A. Hacar (1), A. Palestini (2) ((1) Department of, Astrophysics, Vienna University, (2), MEMOTEF, Sapienza University of Rome)

TL;DR
This study explores how non-isothermal temperature gradients affect the equilibrium structure of filaments in space, revealing they can be more massive and less dense than previously thought under isothermal assumptions.
Contribution
The paper provides new theoretical solutions for non-isothermal filament equilibrium, extending classical models to include observed temperature gradients.
Findings
Non-isothermal filaments can have larger masses per unit length.
Temperature gradients lead to shallower density profiles.
Filaments can remain in equilibrium despite internal temperature variations.
Abstract
The physical properties of the so-called Ostriker isothermal filament (Ostriker 1964) have been classically used as benchmark to interpret the stability of the filaments observed in nearby clouds. However, recent continuum studies have shown that the internal structure of the filaments depart from the isothermality, typically exhibiting radially increasing temperature gradients. The presence of internal temperature gradients within filaments suggests that the equilibrium configuration of these objects should be therefore revisited. The main goal of this work is to theoretically explore how the equilibrium structure of a filament changes in a non-isothermal configuration. We solve the hydrostatic equilibrium equation assuming temperature gradients similar to those derived from observations. We obtain a new set of equilibrium solutions for non-isothermal filaments with both linear and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
