Results 321 to 330 of about 4,469,999 (359)

Flux equipartition in astrophysical plasma turbulence. [PDF]

Sci Adv
Marino R, Xie JH.
europepmc   +1 more source

Tumor ploidy determination in low-pass whole genome sequencing and allelic copy number visualization using the Constellation Plot. [PDF]

Genome Biol
Johnson SH, Smadbeck JB, Zenka RM, Barrett MT, Gaitatzes A, Solanki A, Florio AB, Borad MJ, Cheville JC, Vasmatzis G.   +9 more
europepmc   +1 more source

CryoAlign2: efficient global and local Cryo-EM map retrieval based on parallel-accelerated local spatial structural features. [PDF]

Bioinformatics
Liu Z, He B, Zhang T, Feng C, Zhang F, Yang Z, Han R.   +6 more
europepmc   +1 more source

Mass Supply from Io to Jupiter's Magnetosphere. [PDF]

Space Sci Rev
Roth L, Blöcker A, de Kleer K, Goldstein D, Lellouch E, Saur J, Schmidt C, Strobel DF, Tao C, Tsuchiya F, Dols V, Huybrighs H, Mura A, Szalay JR, Badman SV, de Pater I, Dott AC, Kagitani M, Klaiber L, Koga R, McEwen AS, Milby Z, Retherford KD, Schlegel S, Thomas N, Tseng WL, Vorburger A.   +26 more
europepmc   +1 more source

Organ-resolved lipid mapping in <i>Steatoda nobilis</i> spider model using high-resolution mass spectrometry imaging and Kendrick mass defect analysis. [PDF]

Front Chem
Redureau D, Dunbar JP, La Rocca R, De Monts De Savasse A, Bastiaens Q, Bertrand V, Kune C, Tiquet M, Far J, De Pauw E, Dugon MM, Quinton L.   +11 more
europepmc   +1 more source

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Structure of Molecular Clouds

Astrophysics and Space Science, 2004
This review, far from exhaustive, focuses on the specific properties of molecular clouds in their least condensed phase. Emphasis is placed on their connection with the diffuse medium, their multi-fractal characteristics and the diversity of their small-scale structure, where cold and dense gas may coexist with dilute and warm gas.
Falgarone, Edith, Hily-Blant, Pierre, Levrier, François   +2 more
openaire   +3 more sources

EXTRAGALACTIC MOLECULAR CLOUDS [PDF]

, 2007
We report the results of our study of 436 giant molecular clouds (GMCs) in NGC5128 using dust extinction. The proposed technique allows us toprobe the extinction up to 10 magnitudes in this galaxy. The clump massspectrum, derived by a clumpfind algorithm, is consistent with a powerlaw, dN/dM ∞ M -α, with α = 2.3.
Yuri Beletsky, João Alves
openaire   +2 more sources

Molecular Clouds in the Milky Way

Annual Review of Astronomy and Astrophysics, 2015
Mark H Heyer
exaly   +2 more sources

Interstellar Molecular Clouds

Science, 1986
The interstellar medium in our galaxy contains matter in a variety of states ranging from hot plasma to cold and dusty molecular gas. The molecular phase consists of giant clouds, which are the largest gravitationally bound objects in the galaxy, the primary reservoir of material for the ongoing birth of new stars, and the medium regulating the ...
openaire   +3 more sources