Results 81 to 90 of about 884 (199)

G321.93-0.01: A Rare Site of Multiple Hub-filament Systems with Evidence of Collision and Merging of Filaments

The Astronomical Journal
Hub-filament systems (HFSs) are potential sites of massive star formation (MSF). To understand the role of filaments in MSF and the origin of HFSs, we conducted a multiscale and multiwavelength observational investigation of the molecular cloud G321.93–0.
A. K. Maity, L. K. Dewangan, N. K. Bhadari, Y. Fukui, A. Haj Ismail, O. R. Jadhav, Saurabh Sharma, H. Sano   +7 more
doaj   +1 more source

Intermittency and Anisotropy in the Ionized Interstellar Medium [PDF]

, 2017
The discovery of pulsars was closely followed by the discovery of dispersion and scattering in the interstellar plasma (ionized interstellar medium - IISM).
Barney Rickett
core   +1 more source

The Structure of an 80 Parsec Long Massive Filament

The Astronomical Journal
Using new Institut de Radioastronomie Millimétrique 30 m telescope N _2 H ^+ , C ^18 O J  = 1–0 and Atacama Pathfinder Experiment telescope ^13 CO and C ^18 O J  = 2–1 maps together with archival far-infrared continuum data, and ^12 CO, and ^13 CO J  = 1–
Qian-Ru He, Won-Ju Kim, Gary A. Fuller, Alessio Traficante, Seamus D. Clarke, Yu Gao, Xue-Peng Chen, Min Fang, Ke Wang, En Chen, Tapas Baug, Xiao-Long Wang, Chen Wang, Yong-Xiong Wang   +13 more
doaj   +1 more source

Ionized interstellar froth in irregular galaxies [PDF]

, 1990
The warm interstellar medium of galaxies is a complicated place. It is often full of holes, neutral and ionized loops and shells, and diffuse ionized gas.
Hunter, Deidre A., Gallagher, John S., III   +1 more
core   +1 more source

Bubbles and holes in the interstellar medium [PDF]

, 1996
Studies of the HI in nearby galaxies now clearly begin to show the effects of star formation on the interstellar medium. Holes, filaments, expanding motions and other anomalous velocity signatures are clearly apparent in sensitive observations of the HI ...
vanderHulst, JM; id_orcid
core   +2 more sources

Galactic Large-scale Filaments Resident in Asymmetric Environments: Clues from Cross-filament Profiles of Density and Temperature

The Astrophysical Journal
Large-scale filaments ubiquitously exist in the Galactic interstellar medium, and their radial profiles offer insights into their formation mechanisms. We present a statistical analysis of molecular hydrogen column density (N(H _2 )) and dust temperature
Keyun Su, Ke Wang, Fengwei Xu, N. K. Bhadari   +3 more
doaj   +1 more source

Impact of Supernovae on the Interstellar Medium and the Heliosphere [PDF]

, 2017
The effect of supernovae on their environment is discussed in general and on the heliosphere in particular. It is shown that supernovae generate turbulence on scales of the order of 100 parsecs (pc), which leads to the formation of structures in the ...
M. A. de Avillez, Breitschwerdt, Dieter, de Avillez, Miguel, R. C. Tautz, Tautz, Robert, D. Breitschwerdt   +5 more
core   +1 more source

ACES: The Magnetic Field in Large Filaments in the Galactic Center

The Astrophysical Journal
The Galactic center (GC) is an extreme region of the Milky Way that is host to a complex set of thermal and nonthermal structures. In particular, the GC contains high-density gas and dust that is collectively referred to as the Central Molecular Zone ...
Dylan M. Paré, Zi-Xuan Feng, Yue Hu, Maya A. Petkova, Jack Sullivan, Robin G. Tress, Cara Battersby, Janik Karoly, Alex Lazarian, Dani Lipman, Xing Pan, Marco Donati, Mattia C. Sormani, John Bally, Ashley T. Barnes, Natalie O. Butterfield, Laura Colzi, Christoph Federrath, Pablo Garcia, Adam Ginsburg, Savannah R. Gramze, Anika Schmiedeke, Christian Henkel, Jonathan D. Henshaw, Paul T. Ho, Pei-Ying Hsieh, Izaskun Jimenez-Serra, Ralf S. Klessen, J. M. Diederik Kruijssen, Steven N. Longmore, Xing Lu, Elisabeth A.C. Mills, Álvaro Sánchez-Monge, Daniel L. Walker, Jennifer Wallace, Qizhou Zhang   +35 more
doaj   +1 more source

Wave Structure within HI Filaments at High Galactic Latitude and the Nature of “Clouds” in Interstellar Space [PDF]

Symposium - International Astronomical Union, 1991
Large amplitude waves have been found in the morphology and velocity patterns of several long filaments of HI at high latitude. HI in the filaments is controlled by magnetic fields and the velocity patterns and morphology bear the hallmarks of Alfvén waves.
openaire   +1 more source

Planck intermediate results: XXXIII. Signature of the magnetic field geometry of interstellar filaments in dust polarization maps [PDF]

, 2016
© ESO, 2016.Planck observations at 353 GHz provide the first fully sampled maps of the polarized dust emission towards interstellar filaments and their backgrounds (i.e., the emission observed in the surroundings of the filaments).
Bond J., Bouchet F., Diego J., Boulanger F., Douspis M., Elsner F., Borrill J., Fraisse A., Danese L., Crill B., Forni O., Dickinson C., Arzoumanian D., Christensen P., Davis R., Franceschi E., Ade P., Bersanelli M., Burigana C., Bernard J., Calabrese E., Davies R., De Rosa A., Finelli F., Falgarone E., Bonavera L., Dupac X., Doré O., Eriksen H., Cardoso J., Catalano A., Chamballu A., Clements D., Combet C., Frailis M., Baccigalupi C., Galli S., Bracco A., Delabrouille J., Frejsel A., Couchot F., Cuttaia F., Arnaud M., Berné O., Banday A., Colombo L., Battaner E., De Bernardis P., De Zotti G., Ferrière K., Ducout A., Alves M., Chiang H., Bonaldi A., Bartolo N., Donzelli S., Benoit-Lévy A., Aumont J., Curto A., Bielewicz P., Barreiro R., Enßlin T., Colombi S., Galeotta S., Benabed K., Aghanim N.   +65 more
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