Zobrazeno 1 - 10
of 15 203
pro vyhledávání: '"Bouvier M"'
Autor:
Podio, L., Ceccarelli, C., Codella, C., Sabatini, G., Segura-Cox, D., Balucani, N., Rimola, A., Ugliengo, P., Chandler, C. J., Sakai, N., Svoboda, B., Pineda, J., De Simone, M., Bianchi, E., Caselli, P., Isella, A., Aikawa, Y., Bouvier, M., Caux, E., Chahine, L., Charnley, S. B., Cuello, N., Dulieu, F., Evans, L., Fedele, D., Feng, S., Fontani, F., Hama, T., Hanawa, T., Herbst, E., Hirota, T., Jiménez-Serra, I., Johnstone, D., Lefloch, B., Gal, R. Le, Loinard, L., Liu, H. Baobab, López-Sepulcre, A., Maud, L. T., Maureira, M. J., Menard, F., Miotello, A., Moellenbrock, G., Nomura, H., Oba, Y., Ohashi, S., Okoda, Y., Oya, Y., Sakai, T., Shirley, Y., Testi, L., Vastel, C., Viti, S., Watanabe, N., Watanabe, Y., Zhang, Y., Zhang, Z. E., Yamamoto, S.
Publikováno v:
A&A 688, L22 (2024)
Recent observations suggest that planets formation starts early, in protostellar disks of $\le10^5$ yrs, which are characterized by strong interactions with the environment, e.g., through accretion streamers and molecular outflows. To investigate the
Externí odkaz:
http://arxiv.org/abs/2407.04813
Autor:
Bouvier, M., Viti, S., Behrens, E., Butterworth, J., Huang, K. -Y., Mangum, J. G., Harada, N., Martín, S., Rivilla, V. M., Muller, S., Sakamoto, K., Yoshimura, Y., Tanaka, K., Nakanishi, K., Herrero-Illana, R., Colzi, L., Gorski, M. D., Henkel, C., Humire, P. K., Meier, D. S., van der Werf, P. P., Yan, Y. T.
Publikováno v:
A&A 689, A64 (2024)
Sulphur-bearing species are detected in various environments within Galactic star-forming regions and are particularly abundant in the gas phase of outflows and shocks, and photo-dissociation regions. In this work, we aim to investigate the nature of
Externí odkaz:
http://arxiv.org/abs/2405.08408
Autor:
De Simone, M., Podio, L., Chahine, L., Codella, C., Chandler, C. J., Ceccarelli, C., Lopez-Sepulcre, A., Loinard, L., Svoboda, B., Sakai, N., Johnstone, D., Menard, F., Aikawa, Y., Bouvier, M., Sabatini, G., Miotello, A., Vastel, C., Cuello, N., Bianchi, E., Caselli, P., Caux, E., Hanawa, T., Herbst, E., Segura-Cox, D., Zhang, Z., Yamamoto, S.
Publikováno v:
A&A 686, L13 (2024)
Context. Understanding the connection between outflows, winds, accretion and disks in the inner protostellar regions is crucial for comprehending star and planet formation process. Aims. We aim to we explore the inner 300 au of the protostar IRAS 4A2
Externí odkaz:
http://arxiv.org/abs/2404.19690
Autor:
Sabatini, G., Podio, L., Codella, C., Watanabe, Y., De Simone, M., Bianchi, E., Ceccarelli, C., Chandler, C. J., Sakai, N., Svoboda, B., Testi, L., Aikawa, Y., Balucani, N., Bouvier, M., Caselli, P., Caux, E., Chahine, L., Charnley, S., Cuello, N., Dulieu, F., Evans, L., Fedele, D., Feng, S., Fontani, F., Hama, T., Hanawa, T., Herbst, E., Hirota, T., Isella, A., Jímenez-Serra, I., Johnstone, D., Lefloch, B., Gal, R. Le, Loinard, L., Liu, H. Baobab, López-Sepulcre, A., Maud, L. T., Maureira, M. J., Menard, F., Miotello, A., Moellenbrock, G., Nomura, H., Oba, Y., Ohashi, S., Okoda, Y., Oya, Y., Pineda, J., Rimola, A., Sakai, T., Segura-Cox, D., Shirley, Y., Vastel, C., Viti, S., Watanabe, N., Zhang, Y., Zhang, Z. E., Yamamoto, S.
The origin of the chemical diversity observed around low-mass protostars probably resides in the earliest history of these systems. We aim to investigate the impact of protostellar feedback on the chemistry and grain growth in the circumstellar mediu
Externí odkaz:
http://arxiv.org/abs/2403.18108
Autor:
Vastel, C., Sakai, T., Ceccarelli, C., Jiménez-Serra, I., Alves, F., Balucani, N., Bianchi, E., Bouvier, M., Caselli, P., Chandler, C. J., Charnley, S., Codella, C., De Simone, M., Dulieu, F., Evans, L., Fontani, F., Lefloch, B., Loinard, L., Menard, F., Podio, L., Sabatini, G., Sakai, N., Yamamoto, S.
iCOMs are species commonly found in the interstellar medium. They are believed to be crucial seed species for the build-up of chemical complexity in star forming regions as well as our own Solar System. Thus, understanding how their abundances evolve
Externí odkaz:
http://arxiv.org/abs/2403.07757
Autor:
Butterworth, J., Viti, S., Van der Werf, P. P., Mangum, J. G., Martín, S., Harada, N., Emig, K. L., Muller, S., Sakamoto, K., Yoshimura, Y., Tanaka, K., Herrero-Illana, R., Colzi, L., Rivilla, V. M., Huang, K. Y., Bouvier, M., Behrens, E., Henkel, C., Yan, Y. T., Meier, D. S., Zhou, D.
Publikováno v:
A&A 686, A31 (2024)
Determining the evolution of the CNO isotopes in the interstellar medium (ISM) of starburst galaxies can yield important constraints on the ages of superstar clusters (SSCs), or on other aspects and contributing factors of their evolution. Due to the
Externí odkaz:
http://arxiv.org/abs/2402.10721
Autor:
Mercimek, S., Podio, L., Codella, C., Chahine, L., López-Sepulcre, A., Ohashi, S., Loinard, L., Johnstone, D., Menard, F., Cuello, N., Caselli, P., Zamponi, J., Aikawa, Y., Bianchi, E., Busquet, G., Pineda, J. E., Bouvier, M., De Simone, M., Zhang, Y., Sakai, N., Chandler, C. J., Ceccarelli, C., Alves, F., Durán, A., Fedele, D., Murillo, N., Jiménez-Serra, I., Yamamoto, S.
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
Externí odkaz:
http://arxiv.org/abs/2303.16257
Autor:
Huang, K. -Y., Viti, S., Holdship, J., Mangum, J. G., Martín, S., Harada, N., Muller, S., Sakamoto, K., Tanaka, K., Yoshimura, Y., Herrero-Illana, R., Meier, D. S., Behrens, E., van der Werf, P. P., Henkel, C., García-Burillo, S., Rivilla, V. M., Emig, K. L., Colzi, L., Humire, P. K., Aladro, R., Bouvier, M.
Publikováno v:
A&A 675, A151 (2023)
HNCO and SiO are well known shock tracers and have been observed in nearby galaxies, including the nearby (D=3.5 Mpc) starburst galaxy NGC 253. The simultaneous detection of these two species in regions where the star formation rate is high may be us
Externí odkaz:
http://arxiv.org/abs/2303.12685
Autor:
Chahine, L., López-Sepulcre, A., Podio, L., Codella, C., Neri, R., Mercimek, S., De Simone, M., Caselli, P., Ceccarelli, C., Bouvier, M., Sakai, N., Fontani, F., Yamamoto, S., Alves, F. O., Lattanzi, V., Evans, L., Favre, C.
Publikováno v:
A&A 667, A6 (2022)
Star-forming molecular clouds are characterised by the ubiquity of intertwined filaments. The filaments have been observed in both high- and low-mass star-forming regions, and are thought to split into collections of sonic fibres. The locations where
Externí odkaz:
http://arxiv.org/abs/2209.03696
Autor:
Codella, C., López-Sepulcre, A., Ohashi, S., Chandler, C. J., De Simone, M., Podio, L., Ceccarelli, C., Sakai, N., Alves, F., Durán, A., Fedele, D., Loinard, L., Mercimek, S., Murillo, N., Bianchi, E., Bouvier, M., Busquet, G., Caselli, P., Dulieu, F., Feng, S., Hanawa, T., Johnstone, D., Lefloch, B., Maud, L. T., Moellenbrock, G., Oya, Y., Svoboda, B., Yamamoto, S.
The ALMA 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. Astrochemistry has benefited from imaging interstellar
Externí odkaz:
http://arxiv.org/abs/2206.13339