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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 11/2014, Volume 444, Issue 3, pp. 2507 - 2524
We have carried out a search for filamentary structures in the Taurus molecular cloud using (CO)-C-13 line emission data from the Five Colleges Radio Astronomy... 
ISM: individual objects: Taurus | INITIAL CONDITIONS | COMPLEX | STAR-FORMATION | ISM: structure | PRESTELLAR CORES | stars: formation | radio lines: ISM | ISM: molecules | ASTRONOMY & ASTROPHYSICS | GAS | ACCRETION | ISM: clouds | KINEMATICS
Journal Article
by Abergel, A and Ade, P.A.R and Aghanim, N and Arnaud, M and Ashdown, M and Aumont, J and Baccigalupi, C and Balbi, A and Banday, A.J and Barreiro, R.B and Bartlett, J.G and Battaner, E and Benabed, K and Benoît, A and Bernard, J.-P and Bersanelli, M and Bhatia, R and Bock, J.J and Bonaldi, A and Bond, J.R and Borrill, J and Bouchet, F.R and Boulanger, F and Bucher, M and Burigana, C and Cabella, P and Cardoso, J.-F and Catalano, A and Cayón, L and Challinor, A and Chamballu, A and Chiang, L.-Y and Chiang, C and Christensen, P.R and Clements, D.L and Colombi, S and Couchot, F and Coulais, A and Crill, B.P and Cuttaia, F and Danese, L and Davies, R.D and Davis, R.J and De Bernardis, P and De Gasperis, G and De Rosa, A and De Zotti, G and Delabrouille, J and Delouis, J.-M and Désert, F.-X and Dickinson, C and Dobashi, K and Donzelli, S and Doré, O and Dörl, U and Douspis, M and Dupac, X and Efstathiou, G and Enßlin, T.A and Eriksen, H.K and Finelli, F and Forni, O and Frailis, M and Franceschi, E and Galeotta, S and Ganga, K and Giard, M and Giardino, G and Giraud-Héraud, Y and González-Nuevo, J and Górski, K.M and Gratton, S and Gregorio, A and Gruppuso, A and Guillet, V and Hansen, F.K and Harrison, D and Henrot-Versillé, S and Herranz, D and Hildebrandt, S.R and Hivon, E and Hobson, M and Holmes, W.A and Hovest, W and Hoyland, R.J and Huffenberger, K.M and Jaffe, A.H and Jones, A and Jones, W.C and Juvela, M and Keihänen, E and Keskitalo, R and Kisner, T.S and Kneissl, R and Knox, L and Kurki-Suonio, H and Lagache, G and Lamarre, J.-M and Lasenby, A and Laureijs, R.J and ... and Planck Collaboration
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 536, p. A25
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2014, Volume 444, Issue 3, pp. 2507 - 2524
Journal Article
Astrophysical Journal, ISSN 0004-637X, 03/2016, Volume 819, Issue 1, p. 22
We present observations of (CO)-C-12 J = 1-0, (CO)-C-13 J = 1-0, H I, and all four ground-state transitions of the hydroxyl (OH) radical toward a sharp... 
ISM: clouds | evolution | ISM: individual objects (Taurus) | ISM: molecules | LINE EMISSION | EXCITATION | RATIO | DIFFUSE CLOUDS | COLLISIONS | HYDROGEN | ASTRONOMY & ASTROPHYSICS | MASERS | INTERSTELLAR DUST CLOUDS | MAGNETOHYDRODYNAMIC SHOCKS | Molecular clouds | Gas flow | Emission | Evolution | Radiative transfer | Boundaries | Streams | Radicals | Physics - Astrophysics of Galaxies
Journal Article
Journal Article
ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2012, Volume 760, Issue 2
Young stars form in molecular cores, which are dense condensations within molecular clouds. We have searched for molecular cores traced by (CO)-C-13 J = 1 -> 0... 
850 MICRONS | STAR-FORMATION | SUBMILLIMETER CLUMPS | turbulence | ORIGIN | ISM: individual objects (Taurus) | ISM: molecules | CLUMP DISTRIBUTION | PERSEUS | ASTRONOMY & ASTROPHYSICS | DENSE CORES | ISM: clouds | ORION | INITIAL MASS FUNCTION | EXTINCTION
Journal Article
Astrophysical Journal, ISSN 0004-637X, 12/2012, Volume 760, Issue 2, p. 147
Young stars form in molecular cores, which are dense condensations within molecular clouds. We have searched for molecular cores traced by $^{13}$CO $J=1\to 0$... 
ISM: clouds | ISM: individual objects (Taurus) | ISM: molecules | turbulence Online-only material: color figures | Physics - Astrophysics of Galaxies
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2018, Volume 864, Issue 2, p. 116
Turbulence dissipation is an important process affecting the energy balance in molecular clouds, the birth place of stars. Previously, the rate of turbulence... 
ISM: individual objects (Taurus) | ISM: molecules | ISM: clouds | ISM | STAR-FORMATION | MAGNETOHYDRODYNAMIC TURBULENCE | ASTRONOMY & ASTROPHYSICS | GAS | MAGNETIC-FIELD | GALAXIES | SIMULATIONS | EMISSION | RANGE
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 06/2019, Volume 486, Issue 1, pp. 462 - 485
We present new intensity and polarization observations of the Taurus Molecular Cloud (TMC) region in the frequency range 10-20 GHz with the multifrequency... 
GALACTIC SYNCHROTRON EMISSION | 1420 MHZ | diffuse radiation | radio continuum: ISM | RATIO | MODEL | ALL-SKY SURVEY | radiation mechanisms: general | DUST | IMPACT | ASTRONOMY & ASTROPHYSICS | TO-SELECTIVE EXTINCTION | TEMPLATE | ISM: individual object: Taurus Molecular Cloud, L1527 | COMPONENT SEPARATION | Physics - Astrophysics of Galaxies
Journal Article
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 10/2012, Volume 425, Issue 4, pp. 2641 - 2667
Journal Article
by Xu, Duo and Li, Di
Astrophysical Journal, ISSN 0004-637X, 12/2016, Volume 833, Issue 1, p. 90
We present new observations of all three ground-state transitions of the methylidyne (CH) radical and all four ground-state transitions of the hydroxyl (OH)... 
ISM: clouds | evolution | ISM: individual objects (Taurus) | ISM: molecules | RADIO OBSERVATIONS | EXCITATION | DIFFUSE CLOUDS | INTERSTELLAR CLOUDS | ABUNDANCE | ASTRONOMY & ASTROPHYSICS | CHEMISTRY | EMISSION | EXTINCTION | MAGNETOHYDRODYNAMIC SHOCKS | Physics - Astrophysics of Galaxies
Journal Article
Publications of the Astronomical Society of Japan, ISSN 0004-6264, 12/2013, Volume 66, Issue 6, p. 119
Journal Article