Results 101 to 110 of about 476,181 (204)
Feeding vs Falling. The growth and collapse of molecular clouds in a turbulent interstellar medium
In order to understand the origin of observed molecular cloud properties, it is critical to understand how clouds interact with their environments during their formation, growth and collapse.
Ibáñez-Mejía, Juan C. +11 more
core +1 more source
The Relation between Variances of 3D Density and Its 2D Column Density Revisited
We revisit the relation between the variance of three-dimensional (3D) density ( ${\sigma }_{\rho }^{2}$ ) and that of the projected two-dimensional (2D) column density ( ${\sigma }_{{\rm{\Sigma }}}^{2}$ ) in turbulent media, which is of great importance
Heesun Yoon, Jungyeon Cho
doaj +1 more source
Disclosing Identities in Diffuse Interstellar Bands
The linear isomer of C 3 H 2 has been proposed as the source of broad absorption bands in diffuse interstellar clouds, but it is still being debated.
Benjamin J. McCall, Takeshi Oka
core +1 more source
CO-dark Molecular Gas Traced by HCO+ in the Diffuse Interstellar Medium
A classic problem in the study of the interstellar medium (ISM) is the near-invisibility of molecular hydrogen (H _2 ) in cold environments. Observations of CO emission are typically used to indirectly trace H _2 , but a significant fraction of H _2 in ...
Daniel R. Rybarczyk +4 more
doaj +1 more source
Morphological Evidence for the eROSITA Bubbles Being Giant and Distant Structures
There are two contradictory views of the eROSITA bubbles: either a 10 ^4 pc scale pair of giant bubbles blown by the Galactic center (GC), or a 10 ^2 pc scale local structure coincidentally located in the direction of GC.
Teng Liu +15 more
doaj +1 more source
The abundance of interstellar C60 molecules toward BD+31°643 and other stars
Context. The diffuse interstellar bands (DIBs) at 9577 and 9632 Å are attributed to electronic transitions of the C60+ fullerene ion; thus, its column density in molecular clouds may be inferred.
Rouillé Gaël, Gredel Roland
doaj +1 more source
Interstellar lithium - Differential depletion in diffuse clouds
Les observations de LiId6708 ont conduit a la detection en direction de sept etoiles et a des limites en direction de quinze ...
openaire +1 more source
Compact dusty clouds and efficient H2 formation in diffuse interstellar medium
The formation of compact dusty clouds in diffuse interstellar medium (ISM) has been recently proposed and studied by Tsytovich et al. In the present paper, the effect of the clouds on the rate of H → H2 transition in the ISM is examined.
Caselli, P. +4 more
core +1 more source
Newly computed collisional rate coefficients for the excitation of C _2 in collisions with H _2 , presented recently by Najar & Kalugina, are significantly larger than the values adopted previously in models for the excitation of the C _2 molecule, a ...
David A. Neufeld +9 more
doaj +1 more source
Formaldehyde production in diffuse interstellar clouds [PDF]
Millar, TJ, Duley, W.W., Williams, D.A.
openaire +1 more source

