Results 171 to 180 of about 280,504 (183)

Dark rotors in the late universe. [PDF]

Heliyon, 2015
Mayer FJ.
europepmc   +1 more source

IRC +10 216 in 3-D: morphology of a TP-AGB star envelope. [PDF]

Astron Astrophys, 2018
Guélin M, Patel NA, Bremer M, Cernicharo J, Castro-Carrizo A, Pety J, Fonfría JP, Agúndez M, Santander-García M, Quintana-Lacaci G, Velilla Prieto L, Blundell R, Thaddeus P.   +12 more
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The Comet Interceptor Mission. [PDF]

Space Sci Rev
Jones GH, Snodgrass C, Tubiana C, Küppers M, Kawakita H, Lara LM, Agarwal J, André N, Attree N, Auster U, Bagnulo S, Bannister M, Beth A, Bowles N, Coates A, Colangeli L, Corral van Damme C, Da Deppo V, De Keyser J, Della Corte V, Edberg N, El-Maarry MR, Faggi S, Fulle M, Funase R, Galand M, Goetz C, Groussin O, Guilbert-Lepoutre A, Henri P, Kasahara S, Kereszturi A, Kidger M, Knight M, Kokotanekova R, Kolmasova I, Kossacki K, Kührt E, Kwon Y, La Forgia F, Levasseur-Regourd AC, Lippi M, Longobardo A, Marschall R, Morawski M, Muñoz O, Näsilä A, Nilsson H, Opitom C, Pajusalu M, Pommerol A, Prech L, Rando N, Ratti F, Rothkaehl H, Rotundi A, Rubin M, Sakatani N, Sánchez JP, Simon Wedlund C, Stankov A, Thomas N, Toth I, Villanueva G, Vincent JB, Volwerk M, Wurz P, Wielders A, Yoshioka K, Aleksiejuk K, Alvarez F, Alvarez F, Amoros C, Aslam S, Atamaniuk B, Baran J, Barciński T, Beck T, Behnke T, Berglund M, Bertini I, Bieda M, Binczyk P, Busch MD, Cacovean A, Capria MT, Carr C, Castro Marín JM, Ceriotti M, Chioetto P, Chuchra-Konrad A, Cocola L, Colin F, Crews C, Cripps V, Cupido E, Dassatti A, Davidsson BJR, De Roche T, Deca J, Del Togno S, Dhooghe F, Donaldson Hanna K, Eriksson A, Fedorov A, Fernández-Valenzuela E, Ferretti S, Floriot J, Frassetto F, Fredriksson J, Garnier P, Gaweł D, Génot V, Gerber T, Glassmeier KH, Granvik M, Grison B, Gunell H, Hachemi T, Hagen C, Hajra R, Harada Y, Hasiba J, Haslebacher N, Herranz De La Revilla ML, Hestroffer D, Hewagama T, Holt C, Hviid S, Iakubivskyi I, Inno L, Irwin P, Ivanovski S, Jansky J, Jernej I, Jeszenszky H, Jimenéz J, Jorda L, Kama M, Kameda S, Kelley MSP, Klepacki K, Kohout T, Kojima H, Kowalski T, Kuwabara M, Ladno M, Laky G, Lammer H, Lan R, Lavraud B, Lazzarin M, Le Duff O, Lee QM, Lesniak C, Lewis Z, Lin ZY, Lister T, Lowry S, Magnes W, Markkanen J, Martinez Navajas I, Martins Z, Matsuoka A, Matyjasiak B, Mazelle C, Mazzotta Epifani E, Meier M, Michaelis H, Micheli M, Migliorini A, Millet AL, Moreno F, Mottola S, Moutounaick B, Muinonen K, Müller DR, Murakami G, Murata N, Myszka K, Nakajima S, Nemeth Z, Nikolajev A, Nordera S, Ohlsson D, Olesk A, Ottacher H, Ozaki N, Oziol C, Patel M, Savio Paul A, Penttilä A, Pernechele C, Peterson J, Petraglio E, Piccirillo AM, Plaschke F, Polak S, Postberg F, Proosa H, Protopapa S, Puccio W, Ranvier S, Raymond S, Richter I, Rieder M, Rigamonti R, Ruiz Rodriguez I, Santolik O, Sasaki T, Schrödter R, Shirley K, Slavinskis A, Sodor B, Soucek J, Stephenson P, Stöckli L, Szewczyk P, Troznai G, Uhlir L, Usami N, Valavanoglou A, Vaverka J, Wang W, Wang XD, Wattieaux G, Wieser M, Wolf S, Yano H, Yoshikawa I, Zakharov V, Zawistowski T, Zuppella P, Rinaldi G, Ji H.   +234 more
europepmc   +1 more source

Neutral hydrogen filaments in interstellar media: Are they physical?

Reviews of Modern Plasma Physics
The trending term “filament” is extensively used in the interstellar medium (ISM) and the star formation community, and is believed to be one of the most important objects that gauge molecular cloud and star formation. However, the physical definition of
K. Yuen, K. Ho, C. Law, Avi Chen
semanticscholar   +3 more sources

Properties of interstellar filaments as derived from Herschel observations

, 2014
We present a scenario for filament formation and evolution motivated by recent observational results of nearby molecular clouds. The analysis of more than 250 filaments observed in 7 regions by the Herschel Gould Belt Survey show that the filaments are ...
D. Arzoumanian, P. Andre', N. Peretto, V. Konyves   +3 more
semanticscholar   +2 more sources

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Testing the Theory That Interstellar Filaments Are Formed by the Bennett Pinch With Recent Data

IEEE Transactions on Plasma Science, 2021
Using recent observational data, we here test the theory, first proposed by Carlqvist and Gahm, that astrophysical filaments are formed by the Bennett pinch process.
Y. Nishiyama
semanticscholar   +1 more source

On Interstellar Neutral Hydrogen Associated With an Hα Filament, the Critical Ionization Velocity Effect and the Origin of Filaments

IEEE Transactions on Plasma Science, 2022
Gaussian analysis of neutral hydrogen $\lambda 21$ -cm line (HI) profiles associated with an $\text{H}\alpha $ filament reveal a broad-line underlying component similar to the $\text{H}\alpha $ structure as well as a narrow-line thread along the ...
G. Verschuur, J. Schmelz
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SIMPLIFI -- Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments. I. Magnetically-Guided Accretion onto the DR21 Ridge

We present first results from SIMPLIFI (Study of Interstellar Magnetic Polarization: a Legacy Investigation of Filaments), a SOFIA/HAWC+ $214~\mu\rm{}m$ polarimetric survey of Galactic molecular cloud filaments.
Thushara G. S. Pillai, Jens Kauffmann, J. D. Soler, M. Heyer, Philip C. Myers, L. Fissel, D. Clemens, Koji Sugitani, E. López-Rodríguez, F. Nakamura, Andrea Giannetti, D. Seifried, Paul F. Goldsmith, H. Wiesemeyer, E. Ntormousi, Gabriel A. P. Franco, S. Reissl, K. Menten   +17 more
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Effects of magnetic fields on the formation of Interstellar Filaments through shock-cloud interaction

Astronomy and Computing
D. Gogoi, S.M. Borah, E. Saikia
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