Results 81 to 90 of about 4,494 (233)

Modelling the dust emission from dense interstellar clouds: disentangling the effects of radiative transfer and dust properties [PDF]

, 2012
N. Ysard, M. Juvela, K. Demyk, V. Guillet, A. Abergel, J.-P. Bernard, J. Malinen, C. Mény, L. Montier, D. Paradis, I. Ristorcelli, L. Verstraete   +11 more
openalex   +1 more source

Interstellar planetesimals – II. Radiative instability in dense molecular clouds [PDF]

, 1986
W. M. Napier, C. M. Humphries
openalex   +1 more source

Identification of Galactic H I Counterpart of the Large [O iii] Emission Structure 1 2 Southeast of M31

The Astronomical Journal
Strottner–Drechsler–Sainty Object 1 (SDSO1) is a faint [O iii ] emission nebula spanning 1 $\mathop{.}\limits^{^\circ }5$ , discovered southeast of M31.
Tiantian Liang, Jie Wang, Tao Wang, Haibo Yuan, Ruoyi Zhang, Zhiyu Zhang, Chao-Wei Tsai, Ping Zhou, Xiaohui Sun, Hu Zou, Yingjie Jing, Chen Xu, Zhipeng Hou, Yann Sainty, Marcel Drechsler, Xavier Strottner, Ziming Liu, Qingze Chen, Zerui Liu   +18 more
doaj   +1 more source

A search for naphthalene in diffuse interstellar clouds [PDF]

, 2012
Susana Iglesias-Groth, Jonay González Hernández, A. Manchado   +2 more
openalex   +1 more source

3D Simulation of Interstellar Cloud Collision and Triggered Star Formation [PDF]

, 1987
Mikio Nagasawa, Shoken M. Miyama
openalex   +1 more source

Streaming instabilities in multicomponent interstellar clouds [PDF]

, 2008
Shaukat Ali Shan, H. Saleem, M. Sajid
openalex   +1 more source

Gas Kinematics and Dynamics of Carina Pillars: A Case Study of G287.76-0.87

The Astrophysical Journal
We study the kinematics of a pillar, namely G287.76-0.87, using three rotational lines of ^12 CO(5-4), ^12 CO(8-7), ^12 CO(11-10), and a fine structure line of [O i ] 63 μ m in southern Carina observed by SOFIA/GREAT.
Ngo-Duy Tung, Le Ngoc Tram, Archana Soam, William T. Reach, Edwin Das, Ed Chambers, Blesson Mathew, Heiko Richter   +7 more
doaj   +1 more source

The Transition from Atomic to Molecular Hydrogen in Interstellar Clouds: 21 cm Signature of the Evolution of Cold Atomic Hydrogen in Dense Clouds [PDF]

, 2006
P. F. Goldsmith, Di Li, Marko Krčo
openalex   +1 more source

A sequential acid-base (SAB) mechanism in the interstellar medium: The emergence of cis formic acid in dark molecular clouds [PDF]

, 2023
Juan García de la Concepción, Izaskun Jiménez-Serra, J. C. Corchado, Germán Molpeceres, Antonio Martínez-Henares, V. M. Rivilla, Laura Colzi, J. Martín‐Pintado   +7 more
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Relative Velocities between 13CO Structures within 12CO Molecular Clouds

The Astronomical Journal
Velocity fields of molecular clouds (MCs) can provide crucial information on the merger and split between clouds, as well as their internal kinematics and maintenance, energy injection and redistribution, and even star formation within clouds.
Lixia Yuan, Ji Yang, Xuepeng Chen, Yang Su, Shaobo Zhang, Xin Zhou, Zhiwei Chen, Qing-Zeng Yan, Min Fang, Fujun Du, Yan Sun, Hongchi Wang, Ye Xu   +12 more
doaj   +1 more source