Nonisothermal filaments in equilibrium

Autor(en)
S. Recchi, Alvaro Hacar Gonzalez, A. Palestini
Abstrakt

Context. The physical properties of the so-called Ostriker isothermal

filament have been classically used as a 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. Aims: 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 nonisothermal configuration.

Methods: We solve the hydrostatic equilibrium equation by assuming

temperature gradients similar to those derived from observations.

Results: We obtain a new set of equilibrium solutions for nonisothermal

filaments with both linear and asymptotically constant temperature

gradients. For sufficiently large internal temperature gradients, our

results show that a nonisothermal filament could present significantly

larger masses per unit length and shallower density profiles than the

isothermal filament without collapsing by its own gravity.

Conclusions: We conclude that filaments can reach an equilibrium

configuration under nonisothermal conditions. Detailed studies of both

the internal mass distribution and temperature gradients within

filaments are then needed to judge the physical state of filaments.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Università degli Studi di Roma La Sapienza
Journal
Astronomy & Astrophysics
Band
558
Anzahl der Seiten
5
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361/201321565
Publikationsdatum
10-2013
Peer-reviewed
Ja
ÖFOS 2012
103004 Astrophysik, 103003 Astronomie
Schlagwörter
Link zum Portal
https://ucris.univie.ac.at/portal/de/publications/nonisothermal-filaments-in-equilibrium(be2e9a92-304e-447a-8999-2bc0255a6943).html