Zobrazeno 1 - 10
of 65
pro vyhledávání: '"Mercimek, S."'
Autor:
Codella, C., Podio, L., De Simone, M., Ceccarelli, C., Ohashi, S., Chandler, C. J., Sakai, N., Pineda, J. E., Segura-Cox, D. M., Bianchi, E., Cuello, N., López-Sepulcre, A., Fedele, D., Caselli, P., Charnley, S., Johnstone, D., Zhang, Z. E., Maureira, M. J., Zhang, Y., Sabatini, G., Svoboda, B., Jiménez-Serra, I., Loinard, L., Mercimek, S., Murillo, N., Yamamoto, S.
The ALMA interferometer has played a key role in revealing a new component of the Sun-like star forming process: the molecular streamers, i.e. structures up to thousands of au long funneling material non-axisymmetrically to disks. In the context of t
Externí odkaz:
http://arxiv.org/abs/2402.10258
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:
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
Autor:
Vastel, C., Alves, F., Ceccarelli, C., Bouvier, M., Jimenez-Serra, I., Sakai, T., Caselli, P., Evans, L., Fontani, F., Gal, R. Le, Chandler, C. J., Svoboda, B., Maud, L., Codella, C., Sakai, N., Lopez-Sepulcre, A., Moellenbrock, G., Aikawa, Y., Balucani, N., Bianchi, E., Busquet, G., Caux, E., Charnley, S., Cuello, N., De Simone, M., Dulieu, F., Duran, A., Fedele, D., Feng, S., Francis, L., Hama, T., Hanawa, T., Herbst, E., Hirota, T., Imai, M., Isella, A., Johnstone, D., Lefloch, B., Loinard, L., Maureira, M., Murillo, N. M., Mercimek, S., Mori, S., Menard, F., Miotello, A., Nakatani, R., Nomura, H., Oba, Y., Ohashi, S., Okoda, Y., Ospina-Zamudio, J., Oya, Y., Pineda, J. E., Podio, L., Rimola, A., Cox, D. Segura, Shirley, Y., Testi, L., Viti, S., Watanabe, N., Watanabe, Y., Witzel, A., Xue, C., Zhang, Y., Zhao, B., Yamamoto, S.
Publikováno v:
A&A 664, A171 (2022)
Methanol is a ubiquitous species commonly found in the molecular interstellar medium. It is also a crucial seed species for the building-up of the chemical complexity in star forming regions. Thus, understanding how its abundance evolves during the s
Externí odkaz:
http://arxiv.org/abs/2206.10176
Autor:
Chahine, L., López-Sepulcre, A., Neri, R., Ceccarelli, C., Mercimek, S., Codella, C., Bouvier, M., Bianchi, E., Favre, C., Podio, L., Alves, F. O., Sakai, N., Yamamoto, S.
Publikováno v:
A&A 657, A78 (2022)
Hot corinos are compact regions around solar-mass protostellar objects that are very rich in interstellar complex organic molecules (iCOMs). They are believed to represent the very early phases of our Solar System's birth, which was very likely also
Externí odkaz:
http://arxiv.org/abs/2112.08077
Autor:
Mercimek, S., Codella, C., Podio, L., Bianchi, E., Chahine, L., Bouvier, M., Lopez-Sepulcre, A., Neri, R., Ceccarelli, C.
Publikováno v:
A&A 659, A67 (2022)
Class I protostars are a bridge between Class 0 protostars, and Class II protoplanetary disks. Recent studies show gaps and rings in the dust distribution of disks younger than 1 Myr, suggesting that planet formation may start already at the Class I
Externí odkaz:
http://arxiv.org/abs/2111.07573
Autor:
Garufi, A., Podio, L., Codella, C., Segura-Cox, D., Donckt, M. Vander, Mercimek, S., Bacciotti, F., Fedele, D., Kasper, M., Pineda, J. E., Humphreys, E., Testi, L.
Publikováno v:
A&A 658, A104 (2022)
Planet-forming disks are not isolated systems. Their interaction with the surrounding medium affects their mass budget and chemical content. In the context of the ALMA-DOT program, we obtained high-resolution maps of assorted lines from six disks tha
Externí odkaz:
http://arxiv.org/abs/2110.13820
Autor:
Codella, C., Bianchi, E., Podio, L., Mercimek, S., Ceccarelli, C., Lopez-Sepulcre, A., Bachiller, R., Caselli, P., Sakai, N., Neri, R., Fontani, F., Favre, C., Balucani, N., Lefloch, B., Viti, S., Yamamoto, S.
Publikováno v:
A&A 654, A52 (2021)
Aims: The goal is to obtain a census of S-bearing species using interferometric images, towards SVS13-A, a Class I object associated with a hot corino rich in interstellar complex organic molecules. Methods: We used data at 3mm and 1.4mm obtained wit
Externí odkaz:
http://arxiv.org/abs/2109.01142
Autor:
Codella, C., Podio, L., Garufi, A., Perrero, J., Ugliengo, P., Fedele, D., Favre, C., Bianchi, E., Ceccarelli, C., Mercimek, S., Bacciotti, F., Rygl, K. L. J., Testi, L.
Aims: To trace the radial and vertical spatial distribution of H2CS, a key species of the S-bearing chemistry, in protoplanetary disks. To analyse the observed distributions in light of the H2CS binding energy, in order to discuss the role of thermal
Externí odkaz:
http://arxiv.org/abs/2011.02305