Zobrazeno 1 - 10
of 193
pro vyhledávání: '"Nguyen Luong, Q."'
Autor:
Nguyen-Luong, Q., Adam, R., Ade, P., Ajeddig, H., André, P., Artis, E., Aussel, H., Beelen, A., Benoît, A., Berta, S., Bing, L., Bourrion, O., Calvo, M., Catalano, A., De Petris, M., Désert, F. -X., Doyle, S., Driessen, E. F. C., Ejlali, G., Gomez, A., Goupy, J., Hanser, C., Katsioli, S., Kéruzoré, F., Kramer, C., Ladjelate, B., Lagache, G., Leclercq, S., Lestrade, J. -F., Macías-Pérez, J. F., Madden, S. C., Maury, A., Mauskopf, P., Mayet, F., Monfardini, A., Moyer-Anin, A., Muñoz-Echeverría, M., Perotto, L., Pisano, G., Ponthieu, N., Revéret, V., Rigby, A. J., Ritacco, A., Romero, C., Roussel, H., Ruppin, F., Schuster, K., Sievers, A., Tucker, C., Zylka, R., Bacmann, A., Duong-Tuan, A., Peretto, N., Rigby, A.
To understand the evolution of dust properties in molecular clouds in the course of the star formation process, we constrain the changes in the dust emissivity index from star-forming filaments to prestellar and protostellar cores to T Tauri stars. U
Externí odkaz:
http://arxiv.org/abs/2310.16526
Autor:
Towner, A. P. M., Ginsburg, A., Dell'Ova, P., Gusdorf, A., Bontemps, S., Csengeri, T., Galván-Madrid, R., Louvet, F. K., Motte, F., Sanhueza, P., Stutz, A. M., Bally, J., Baug, T., Chen, H. R. V., Cunningham, N., Fernández-López, M., Liu, H. -L., Lu, X., Nony, T., Valeille-Manet, M., Wu, B., Álvarez-Gutiérrez, R. H., Bonfand, M., Di Francesco, J., Nguyen-Luong, Q., Olguin, F., Whitworth, A. P.
We present a catalog of 315 protostellar outflow candidates detected in SiO J=5-4 in the ALMA-IMF Large Program, observed with ~2000 au spatial resolution, 0.339 km/s velocity resolution, and 2-12 mJy/beam (0.18-0.8 K) sensitivity. We find median out
Externí odkaz:
http://arxiv.org/abs/2310.13125
Autor:
Neralwar, K. R., Colombo, D., Duarte-Cabral, A., Urquhart, J. S., Mattern, M., Wyrowski, F., Menten, K. M., Barnes, P., Sanchez-Monge, A., Rigby, A. J., Mazumdar, P., Eden, D., Csengeri, T., Dobbs, C. L., Veena, V. S., Neupane, S., Henning, T., Schuller, F., Leurini, S., Wienen, M., Yang, A. Y., Ragan, S. E., Medina, S., Nguyen-Luong, Q.
Publikováno v:
A&A 664, A84 (2022)
The Structure, Excitation, and Dynamics of the Inner Galactic InterStellar Medium (SEDIGISM) survey has produced high (spatial and spectral) resolution $^{13}$CO (2-1) maps of the Milky Way. It has allowed us to investigate the molecular interstellar
Externí odkaz:
http://arxiv.org/abs/2205.02253
Autor:
Neralwar, K. R., Colombo, D., Duarte-Cabral, A., Urquhart, J. S., Mattern, M., Wyrowski, F., Menten, K. M., Barnes, P., Sanchez-Monge, A., Beuther, H., Rigby, A. J., Mazumdar, P., Eden, D., Csengeri, T., Dobbs, C. L., Veena, V. S., Neupane, S., Henning, T., Schuller, F., Leurini, S., Wienen, M., Yang, A. Y., Ragan, S. E., Medina, S., Nguyen-Luong, Q.
Publikováno v:
A&A 663, A56 (2022)
We present one of the very first extensive classifications of a large sample of molecular clouds based on their morphology. This is achieved using a recently published catalogue of 10663 clouds obtained from the first data release of the SEDIGISM sur
Externí odkaz:
http://arxiv.org/abs/2203.02504
Autor:
Schuller, F., Urquhart, J. S., Csengeri, T., Colombo, D., Duarte-Cabral, A., Mattern, M., Ginsburg, A., Pettitt, A. R., Wyrowski, F., Anderson, L., Azagra, F., Barnes, P., Beltran, M., Beuther, H., Billington, S., Bronfman, L., Cesaroni, R., Dobbs, C., Eden, D., Lee, M. -Y., Medina, S. -N. X., Menten, K. M., Moore, T., Montenegro-Montes, F. M., Ragan, S., Rigby, A., Riener, M., Russeil, D., Schisano, E., Sanchez-Monge, A., Traficante, A., Zavagno, A., Agurto, C., Bontemps, S., Finger, R., Giannetti, A., Gonzalez, E., Hernandez, A. K., Henning, T., Kainulainen, J., Kauffmann, J., Leurini, S., Lopez, S., Mac-Auliffe, F., Mazumdar, P., Molinari, S., Motte, F., Muller, E., Nguyen-Luong, Q., Parra, R., Perez-Beaupuits, J. -P., Schilke, P., Schneider, N., Suri, S., Testi, L., Torstensson, K., Veena, V. S., Venegas, P., Wang, K., Wienen, M.
The SEDIGISM (Structure, Excitation and Dynamics of the Inner Galactic Interstellar Medium) survey used the APEX telescope to map 84 deg^2 of the Galactic plane between l = -60 deg and l = +31 deg in several molecular transitions, including 13CO(2-1)
Externí odkaz:
http://arxiv.org/abs/2012.01527
Autor:
Duarte-Cabral, A., Colombo, D., Urquhart, J. S., Ginsburg, A., Russeil, D., Schuller, F., Anderson, L. D., Barnes, P. J., Beltran, M. T., Beuther, H., Bontemps, S., Bronfman, L., Csengeri, T., Dobbs, C. L., Eden, D., Giannetti, A., Kauffmann, J., Mattern, M., Medina, S. -N. X., Menten, K. M., Lee, M. -Y., Pettitt, A. R., Riener, M., Rigby, A. J., Trafficante, A., Veena, V. S., Wienen, M., Wyrowski, F., Agurto, C., Azagra, F., Cesaroni, R., Finger, R., Gonzalez, E., Henning, T., Hernandez, A. K., Kainulainen, J., Leurini, S., Lopez, S., Mac-Auliffe, F., Mazumdar, P., Molinari, S., Motte, F., Muller, E., Nguyen-Luong, Q., Parra, R., Perez-Beaupuits, J. -P., Montenegro-Montes, F. M., Moore, T. J. T., Ragan, S. E., Sanchez-Monge, A., Sanna, A., Schilke, P., Schisano, E., Schneider, N., Suri, S., Testi, L., Torstensson, K., Venegas, P., Wang, K., Zavagno, A.
We use the 13CO(2-1) emission from the SEDIGISM high-resolution spectral-line survey of the inner Galaxy, to extract the molecular cloud population with a large dynamic range in spatial scales, using the SCIMES algorithm. This work compiles a cloud c
Externí odkaz:
http://arxiv.org/abs/2012.01502
Autor:
Nguyen-Luong, Q., Anderson, L. D., D., L., Motte, F., Kim, Kee-Tae, Schilke, P., Carlhoff, P., Beuther, H., Schneider, N., Didelon, P., Kramer, C., Louvet, F., Nony, T., Bihr, S., Rugel, M., Soler, J., Wang, Y., Bronfman, L., Simon, R., Menten, K. M., Wyrowski, F., Walmsley, M.
We report the first map of large-scale (10 pc in length) emission of millimeter-wavelength hydrogen recombination lines (mm-RRLs) toward the giant H II region around the W43-Main young massive star cluster (YMC). Our mm-RRL data come from the IRAM 30
Externí odkaz:
http://arxiv.org/abs/2009.03307
Autor:
Nguyen-Luong, Q.1,2 qnguyen@aup.edu, Adam, R.3, Ade, P.4, Ajeddig, H.2, André, P.2, Artis, E.5,6, Aussel, H.2, Beelen, A.7, Benoît, A.8, Berta, S.9, Bing, L.7, Bourrion, O.5, Calvo, M.8, Catalano, A.5, De Petris, M.10, Désert, F.-X.11, Doyle, S.4, Driessen, E.F.C.9, Ejlali, G.12, Gomez, A.13
Publikováno v:
EPJ Web of Conferences. 3/28/2024, Vol. 293, p1-7. 7p.
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Autor:
Saral, G., Hora, J. L., Audard, M., Koenig, X. P., Martínez-Galarza, J. R., Motte, F., Nguyen-Luong, Q., Saygac, A. T., Smith, H. A.
We present the results of our investigation of the star-forming complexes W51 and W43, two of the brightest in the first Galactic quadrant. In order to determine the young stellar object (YSO) populations in W51 and W43 we used color-magnitude relati
Externí odkaz:
http://arxiv.org/abs/1703.02771