Zobrazeno 1 - 10
of 48
pro vyhledávání: '"C J Chandler"'
Autor:
S Mercimek, L Podio, C Codella, L Chahine, A López-Sepulcre, S Ohashi, L Loinard, D Johnstone, F Menard, N Cuello, P Caselli, J Zamponi, Y Aikawa, E Bianchi, G Busquet, J E Pineda, M Bouvier, M De Simone, Y Zhang, N Sakai, C J Chandler, C Ceccarelli, F Alves, A Durán, D Fedele, N Murillo, I Jiménez-Serra, S Yamamoto
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 522:2384-2392
More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostellar stage. We report continuum and C$^{18}$O (2-1) observations of the
Autor:
C Codella, A López-Sepulcre, S Ohashi, C J Chandler, M De Simone, L Podio, C Ceccarelli, N Sakai, F Alves, A Durán, D Fedele, L Loinard, S Mercimek, N Murillo, Y Zhang, E Bianchi, M Bouvier, G Busquet, P Caselli, F Dulieu, S Feng, T Hanawa, D Johnstone, B Lefloch, L T Maud, G Moellenbrock, Y Oya, B Svoboda, S Yamamoto
C. Codella et al.
The ALMA (Atacama Large Millimeter Array) interferometer, with its unprecedented combination of high sensitivity and high angular resolution, allows for (sub-)mm wavelength mapping of protostellar systems at Solar system scales
The ALMA (Atacama Large Millimeter Array) interferometer, with its unprecedented combination of high sensitivity and high angular resolution, allows for (sub-)mm wavelength mapping of protostellar systems at Solar system scales
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b9a09c688b20bd9af78479e4d6735a8b
http://arxiv.org/abs/2206.13339
http://arxiv.org/abs/2206.13339
Autor:
G. Guidi, A. Isella, L. Testi, C. J. Chandler, H. B. Liu, H. M. Schmid, G. Rosotti, C. Meng, J. Jennings, J. P. Williams, J. M. Carpenter, I. de Gregorio-Monsalvo, H. Li, S. F. Liu, S. Ortolani, S. P. Quanz, L. Ricci, M. Tazzari
Publikováno v:
Astronomy & Astrophysics, 664:A137
Astronomy & Astrophysics, 664
Astronomy & Astrophysics, 664
Context. Observations at millimeter wavelengths of bright protoplanetary disks have shown the ubiquitous presence of structures such as rings and spirals in the continuum emission. The derivation of the underlying properties of the emitting material
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2db1014d09fa7d9258600a2c7f731532
https://hdl.handle.net/1887/3561748
https://hdl.handle.net/1887/3561748
Autor:
C. Vastel, F. Alves, C. Ceccarelli, M. Bouvier, I. Jiménez-Serra, T. Sakai, P. Caselli, L. Evans, F. Fontani, R. Le Gal, C. J. Chandler, B. Svoboda, L. Maud, C. Codella, N. Sakai, A. Lόpez-Sepulcre, G. Moellenbrock, Y. Aikawa, N. Balucani, E. Bianchi, G. Busquet, E. Caux, S. Charnley, N. Cuello, M. De Simone, F. Dulieu, A. Durân, D. Fedele, S. Feng, L. Francis, T. Hama, T. Hanawa, E. Herbst, T. Hirota, M. Imai, A. Isella, D. Johnstone, B. Lefloch, L. Loinard, M. Maureira, N. M. Murillo, S. Mercimek, S. Mori, F. Menard, A. Miotello, R. Nakatani, H. Nomura, Y. Oba, S. Ohashi, Y. Okoda, J. Ospina-Zamudio, Y. Oya, J. E. Pineda, L. Podio, A. Rimola, D. Segura Cox, Y. Shirley, L. Testi, S. Viti, N. Watanabe, Y. Watanabe, A. Witzel, C. Xue, Y. Zhang, B. Zhao, S. Yamamoto
Publikováno v:
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2022, 664 (1), pp.171. ⟨10.1051/0004-6361/202243414⟩
Astronomy & Astrophysics, 664:A171
Astronomy and Astrophysics-A&A, 2022, 664 (1), pp.171. ⟨10.1051/0004-6361/202243414⟩
Astronomy & Astrophysics, 664:A171
C. Vastel et al.
[Aims] Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the build-up of chemical complexity in star forming regions. Thus, understanding how its abundanc
[Aims] Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the build-up of chemical complexity in star forming regions. Thus, understanding how its abundanc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7e8ca2608cb4103b7f1a99218f4fa716
https://hdl.handle.net/1887/3514992
https://hdl.handle.net/1887/3514992
Publikováno v:
The Astrophysical Journal. 698:1165-1173
We have used the Very Large Array (VLA) at 7 mm wavelength to image five rotational transitions (J = 1 − 0) from three SiO isotopologues towards Orion BN/KL: 28 SiO v = 0,1,2; and 29 SiO and 30 SiO v = 0. For the first time, we have mapped the 29 S
Autor:
R. C. Bolton, C. J. Chandler, G. Cotter, T. J. Pearson, G. G. Pooley, A. C. S. Readhead, J. M. Riley, E. M. Waldram
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 370:1556-1564
We present Australia Telescope Compact Array (ATCA) HI imaging of the edge-on galaxy NGC 1596, which was recently found to have counter-rotating ionized gas in its center (
Publikováno v:
Symposium - International Astronomical Union. 221:155-160
High-mass star formation is not well understood chiefly because examples are deeply embedded, relatively distant, and crowded with sources of emission. Using VLA and VLBA observations of H2O and SiO maser emission, we have mapped in detail the struct
Autor:
K. Björkegren, C. Bergmark, U. de Faire, M. Azam Mansoor, A. Svardal, A. G. Bostom, R. Roubenoff, P. Dellaripa, M. R. Nadeau, P. Sutherland, P. W. F. Wilson, P. F. Jacques, J. Selhub, I. H. Rosenberg, J. T. Brosnan, B. Hall, D. Shemin, K. L. Lapane, R. R. Williams, R. C. Ellison, G. J. Cuskelly, H. McNulty, J. J. Strain, J. M. McPartlin, J. M. Scott, B. Chadefaux-Vekemans, M. Coudé, J. Aupetit, P. Kamoun, B. Aral, M. T. Zabot, R. Calaf, O. Ghiringelli, A. Barlatier, P. Charpiot, P. H. Rolland, D. Garçon, T. Augier, C. Chareyre, A. Chango, F. Hodez, H. Tronel, G. Nuel, F. Michel, S. Frémont, L. Méjean, J. P. Nicolas, M. Candito, P. Chambon, P. Gibelin, J. Amsellem, M. Baudouy, P. Morand, D. Pringuey, V. Aubin-Brunet, F. Beaulieu, G. Darcourt, P. Bedoucha, H. Alchaar, M. Chatel, H. W. de Valk, R. van der Griend, M. K. G. van Eeden, E. de Groot, M. Duran, J. A. M. Smeitink, J. B. C. de Klerk, D. Wittebol-Post, M. -O. Rolland, F. J. L. M. Haas, O. J. A. Th. Meuwissen, J. D. Banga, B. T. Poll-The, J. I. P. de Vries, G. A. Dekker, H. P. van Geijn, P. C. Huigens, C. Jakobs, B. M. E. von Blomberg, R. Deulofeu, M. Giralt, C. Aibar, C. Bauchet, A. M. Ballesta, G. Varela, N. Vila, A. Chamorro, F. J. Casals, J. Diaz Cremades, L. Daly, R. Meleady, I. Graham, M. den Heijer, I. A. Brouwer, W. B. J. Gerrits, G. M. J. Bos, H. J. Blom, T. Koster, J. P. Vandenbroucke, E. Briët, F. R. Rosendaal, G. Fischer, C. Behrend, P. Bartholmes, I. Fermo, R. Paroni, S. Vigano, A. D’Angelo, D. G. Franken, G. H. J. Boers, B. C. J. Hamel, J. H. J. Ruijs, A. Tangerman, A. B. Guttormsen, P. M. Ueland, H. Refsum, E. Svarstad, W. Gao, E. Goldman, H. Jakubowski, G. Sebastio, M. P. Sperandeo, R. de Franchis, G. Andria, T. A. Garrow, J. Hladovec, Z. Sommerova, A. Písariková, C. H. Halsted, J. Villanueva, C. J. Chandler, S. P. Stabler, R. H. Allen, L. Muskhelishvili, S. J. James, L. Poirer, D. W. Jacobsen, S. R. Savon, P. E. DiCorleto, D. Jourdheuil-Rahmani, E. Joosten, R. Riezler, R. Allen, T. Marquardt, K. Ullrich, E. Harms, H. G. Koch, S. Evers, K. H. Grotemeyer, L. Vogelpohl, A. von Eckardstein, T. Deufel, J. Kraus, V. Kozich, M. Janosik, J. Sokolová, G. Bukovská, J. P. Kraus, L. A. J. Kluitmans, L. P. van den Heuvel, E. Stevens, J. M. F. Trubels, B. A. van Oost, S. Kittner, R. Macko, J. R. Hebel, J. Rohr, M. R. Malinow, B. Upson, D. Buchholz, C. Earley, C. Johnson, T. R. Price, J. Rosario, M. Sloan, B. Stern, R. Wityk, M. Wozniak, R. Sherwin, P. Stolley, L. Kluijtmans, L. van den Heuvel, F. Trijbels, H. Blom, G. Boers, B. van Oost, R. Rozen, F. Löhrer, C. Angst, B. Fowler, M. Zaugg, F. Brunner, W. E. Haefeli, B. Nedrebø, U. -B. Ericsson, E. A. Lien, J. London, E. Paly, V. Paul, D. Paris, J. F. Chassé, J. Møller, K. Rasmussen, P. Verhoef, K. E. McMartin, T. J. Phifer, J. S. Alexander, M. Middlebrooks, L. E. Childress, S. Fremont, F. Felden, B. Guerci, C. Creton, P. Drouin, G. P. Oakley, P. R. P. Elias, A. C. Hann, C. G. Curtis, F. A. Rose, N. Tudball, F. Parrot-Roulaud, C. Cochet, B. Catargi, F. Leprat, J. -L. Latapie, A. F. Perna, N. G. De Santo, D. Ingrosso, P. Galletti, V. Zappia, G. Sassoust, P. Boissieras, A. K. Majors, L. A. Ehrhart, E. H. Pezacka, I. J. Perry, R. W. Morris, S. B. Ebrahim, A. G. Shaper, K. Pietrzik, J. Dierkes, M. Kroesen, P. Bung, J. Moller, A. Remacha, F. Garcia-Die, J. Cadafalch, H. J. Barceló, H. Parellada, B. Regland, C. -G. Gottfries, M. Andersson, J. Bagby, L. -E. Dyrehag, L. Abrahamsson, E. Ronge, B. Kjellman, P. Frosst, B. Christensen, P. Goyette, D. S. Rosenblatt, J. Genest, B. Riedel, A. M. Svardal, J. Silberberg, R. Crooks, J. Fryer, C. Ray, X. W. Guo, L. Xie, N. Dudman, X. Guo, B. Smith, D. Kohlman-Trigoboff, S. Simsir, A. J. C. Strydom, E. Schlüssel, G. Preibisch, E. F. E. Elstner, S. Pütter, M. D. E. H. Spuijbroek, T. A. W. Goddijn-Wessel, M. G. A. J. Wouters, E. F. v. d. Molen, R. P. M. Steegers-Theunissen, J. M. F. Trijbels, C. M. G. Thomas, T. K. A. B. Eskes, M. Y. Tsai, N. Hanson, N. Key, K. Schwichtenberg, U. Garg, L. Todesco, N. Pollaert, B. Thorand, M. Hages, W. Holzgreve, M. J. van der Mooren, L. A. Schellekens, R. Rolland, N. v. d. Put, L. v. d. Heuvel, T. Eskes, R. Steegers-Theunissen, E. Mariman, M. d. Heyer, R. Daher, F. Van Lente, A. B. Vilkovsky, I. V. Maev, E. L. Richter, M. D. Kirnus, G. Varela-Moreiras, E. Alonso-Aperte, M. Rubio, M. Gassó, L. Alvarez, J. Caballeria, J. Rodés, J. M. Mato, L. A. G. J. M. van Aerts, J. H. J. Copius Peereboom-Stegeman, J. Noordhoek, L. P. v. d. Heuvel, L. A. H. Monnens, C. van Guidener, M. J. F. M. Janssen, J. Surachno, C. D. A. Stehouwer, M. van den Berg, E. Bierdrager, J. A. Rauwerda, B. Wilcken, J. Hammond, C. J. C. M. Hamilton, G. F. Borm, H. Wang, J. -C. Tsai, M. A. Perrella, M. Yoshizumi, N. E. S. Sibinga, E. Haber, T. H. -T. Chang, R. Schlegel, M. -E. Lee, J. Woodside, D. McMaster, J. Yarnell, I. Young, C. Mercer, K. Byrne, A. Evans, F. Gey, X. M. Gao, G. Dougan, P. Wordsworth, A. McMichael, P. B. Young, D. G. Kennedy, A. M. Molloy, P. Ward, E. Naughten, S. Cahalane, D. Murphy, P. Mayne, P. Chauveau, P. Jungers, D. Z. B. van Asselt, G. M. de Wild, W. A. van Staveren, W. H. L. Hoefnagels, M. Naruszewicz, A. Staniewicz, K. Dziewanowski, J. Evrovski, D. E. C. Cole, Michael Callaghan, A. Lindgren, L. Brattström, B. Hultberg, C. H. Hennekens, W. C. Willett, M. J. Stampfer, F. Frantzen, E. Sundrehagen, F. J. Kok, J. M. Gaziano, R. D. Reynolds, R. -J. Hsu, B. Shane, K. Robinson, K. Kottke-Marchant, R. Green, A. Gupta, D. Jacobsen, E. Mayer, D. Miller, K. Marchant, R. Greene, Y. -Y. Chong, M. Gupta, C. A. Sheppard, R. G. Matthews, H. A. C. M. Kruyssen, J. C. M. Witteman, C. Boushey, S. Beresford, G. Omenn, A. G. Motulsky, O. Nygard, S. E. Vollset, G. Kvale, I. Stensvold, T. Fiskerstrand, K. H. Bugge, A. Oshaug, C. H. Bjønnes, J. T. Wu, L. L. Wu, L. W. Wilson
Publikováno v:
Irish Journal of Medical Science. 164:56-83
Publikováno v:
Astrophysics and Space Science. 212:191-195
We investigate the question of disk formation during the protostar phase. We build on the results of Keene and Masson (1990) whose analysis of L1551 showed the millimeter continuum emission comes from both an unresolved circumstellar component, i.e.,
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 261:694-704
We have mapped the young star formation region DR21(OH) in the J=2-1 and 1-0 transitions of CS and C 34 S, and have obtained spectra with high signal-to-noise ratios towards the three main continuum sources within the core. We find that the CS emissi