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by Ade, P.A.R and Aghanim, N and Alves, M.I.R and Arnaud, M and Arzoumanian, D and Ashdown, M and Aumont, J and Baccigalupi, C and Banday, A.J and Barreiro, R.B and Bartolo, N and Battaner, E and Benabed, K and Benoît, A and Benoit-Lévy, A and Bernard, J.-P and Bersanelli, M and Bielewicz, P and Bock, J.J and Bonavera, L and Bond, J.R and Borrill, J and Bouchet, F.R and Boulanger, F and Bracco, A and Burigana, C and Calabrese, E and Cardoso, J.-F and Catalano, A and Chiang, H.C and Christensen, P.R and Colombo, L.P.L and Combet, C and Couchot, F and Crill, B.P and Curto, A and Cuttaia, F and Danese, L and Davies, R.D and Davis, R.J and De Bernardis, P and De Rosa, A and De Zotti, G and Delabrouille, J and Dickinson, C and Diego, J.M and Dole, H and Donzelli, S and Doré, O and Douspis, M and Ducout, A and Dupac, X and Efstathiou, G and Elsner, F and Enßlin, T.A and Eriksen, H.K and Falceta-Gonçalves, D and Falgarone, E and Ferrière, K and Finelli, F and Forni, O and Frailis, M and Fraisse, A.A and Franceschi, E and Frejsel, A and Galeotta, S and Galli, S and Ganga, K and Ghosh, T and Giard, M and Gjerløw, E and González-Nuevo, J and Górski, K.M and Gregorio, A and Gruppuso, A and Gudmundsson, J.E and Guillet, V and Harrison, D.L and Helou, G and Hennebelle, P and Henrot-Versillé, S and Hernández-Monteagudo, C and Herranz, D and Hildebrandt, S.R and Hivon, E and Holmes, W.A and Hornstrup, A and Huffenberger, K.M and Hurier, G and Jaffe, A.H and Jaffe, T.R and Jones, W.C and Juvela, M and Keihänen, E and Keskitalo, R and Kisner, T.S and Knoche, J and Kunz, M and Kurki-Suonio, H and Lagache, G and ... and Planck Collaboration and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Astronomy and Astrophysics, ISSN 0004-6361, 02/2016, Volume 586, p. A138
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 12/2009, Volume 508, Issue 3, pp. L35 - L38
Context. Probability distribution of densities is a fundamental measure of molecular cloud structure, containing information on how the material arranges... 
Evolution | ISM: clouds | Stars: formation | ISM: structure | Dust, extinction | DECAYING TURBULENCE | DISTANCE | evolution | COLUMN DENSITY | STAR-FORMING REGIONS | stars: formation | DARK CLOUDS | dust, extinction | ASTRONOMY & ASTROPHYSICS | SIMULATIONS | INITIAL MASS FUNCTION | NEAR-INFRARED OBSERVATIONS | PROBABILITY-DISTRIBUTION | EXTINCTION
Journal Article
Astrophysical Journal, ISSN 0004-637X, 09/2011, Volume 738, Issue 1, p. 34
Journal Article
The Astrophysical Journal, ISSN 0004-637X, 10/2011, Volume 740, Issue 1, p. 45
We present a study of dense molecular gas kinematics in 17 nearby protostellar systems using single-dish and interferometric molecular line observations. The... 
stars: formation | radio lines: ISM | ISM: molecules | ISM: kinematics and dynamics | SPITZER C2D SURVEY | LOW-MASS PROTOSTARS | INTERSTELLAR AMMONIA | YOUNG STELLAR OBJECTS | HH 211 | DARK CLOUDS | ASTRONOMY & ASTROPHYSICS | DENSE CORES | VLBA DETERMINATION | EVOLVED STARLESS CORE | SUBMILLIMETER CONTINUUM OBSERVATIONS
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2011, Volume 530, p. A64
We present an analysis of the large-scale molecular cloud structure and of the stability of clumpy structures in nearby molecular clouds. In our recent work,... 
stars: formation | ISM: clouds | dust, extinction | evolution | ISM: structure | 2D OBSERVATIONS | STAR-FORMATION | INTERSTELLAR CLOUDS | OPHIUCHI MAIN CLOUD | COLUMN-DENSITY | FIELD EXTINCTION MAPS | ASTRONOMY & ASTROPHYSICS | INITIAL MASS FUNCTION | NEAR-INFRARED OBSERVATIONS | PROBABILITY-DISTRIBUTION | SUPERSONIC TURBULENCE
Journal Article
by Adam, R and Ade, PAR and Aghanim, N and Alves, MIR and Arnaud, M and Arzoumanian, D and Ashdown, M and Aumont, J and Baccigalupi, C and Banday, AJ and Barreiro, RB and Bartolo, N and Battaner, E and Benabed, K and Benoit-Levy, A and Bernard, JP and Bersanelli, M and Bielewicz, P and Bonaldi, A and Bonavera, L and Bond, JR and Borrill, J and Bouchet, FR and Boulanger, F and Bracco, A and Burigana, C and Butler, RC and Calabrese, E and Cardoso, JF and Catalano, A and Chamballu, A and Chiang, HC and Christensen, PR and Colombi, S and Colombo, LPL and Combet, C and Couchot, F and Crill, BP and Curto, A and Cuttaia, F and Danese, L and Davies, RD and Davis, RJ and de Bernardis, P and de Rosa, A and de Zotti, G and Delabrouillel, J and Dickinson, C and Diego, JM and Dole, H and Donzelli, S and Dore, O and Douspis, M and Ducout, A and Dupac, X and Efstathiou, G and Elsner, F and Ensslin, TA and Eriksen, HK and Falgarone, E and Ferriere, K and Finelli, F and Forni, O and Frailis, M and Fraisse, AA and Franceschi, E and Frejse, A and Galeotta, S and Gai, S and Ganga, K and Ghosh, T and Giard, M and Gjerlow, E and Gonzalez-Nuevo, J and Gorski, KM and Gregorio, A and Gruppuso, A and Guillet, V and Hansen, K and Hanson, D and Harrison, DL and Henrot-Versille, S and Hernandez-Monteagudo, C and Herranz, D and Hildebrandt, SR and Hivon, E and Hobson, M and Holmes, WA and Hovest, W and Huffenberger, KM and Hurier, G and Jaffe, AH and Jaffe, TR and Jones, WC and Juvela, M and Keihanen, E and Keskitalo, R and Kisner, TS and Kneiss, R and Knoche, J and ... and Planck Collaboration and Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 02/2016, Volume 586, p. A135
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 03/2019, Volume 485, Issue 4, pp. 4509 - 4528
We perform ideal magnetohydrodynamics high-resolution adaptive mesh refinement simulations with driven turbulence and self-gravity and find that long... 
ISM:Evolution | ISM: Magnetic fields | ISM: Kinematics and dynamics | turbulence | ISM: Clouds | methods: Numerical | HELICAL FIELDS | GRAVITATIONAL-INSTABILITY | ISM: evolution | ASTRONOMY & ASTROPHYSICS | ISM: kinematics and dynamics | GAS | ISM: clouds | SIMULATIONS | methods: numerical | FRAGMENTATION | ISM: magnetic fields
Journal Article
ASTRONOMY & ASTROPHYSICS, ISSN 1432-0746, 07/2019, Volume 628, p. A6
Context. Sagittarius B2 (north) is a chemically rich, high-mass star-forming region located within the giant molecular cloud complex Sgr B2 in the central... 
stars: formation | W33A | radio lines: ISM | STAR | ASTRONOMY & ASTROPHYSICS | ISM: kinematics and dynamics | ISM: individual objects: SgrB2(N) | stars: massive | techniques: high angular resolution
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2007, Volume 465, Issue 2, pp. 431 - 443
Journal Article