Zobrazeno 1 - 10
of 7 197
pro vyhledávání: '"Alves F"'
Autor:
Vilares-Morgado R, Correia V, Ferreira AM, Alves F, Melo AB, Estrela-Silva S, Araújo J, Tavares-Ferreira J, Silva M, Rocha-Sousa A, Carneiro A, Barbosa-Breda J
Publikováno v:
Clinical Ophthalmology, Vol Volume 17, Pp 3613-3627 (2023)
Rodrigo Vilares-Morgado,1,2 Vera Correia,3 Ana Margarida Ferreira,1 Flávio Alves,1 António Benevides Melo,1,3 Sérgio Estrela-Silva,1,3 Joana Araújo,1,3 João Tavares-Ferreira,1,3 Marta Silva,1 Amândio Rocha-Sousa,1,2 Angela Carneiro,1,2 João Ba
Externí odkaz:
https://doaj.org/article/80f7b32a3f4144cbad2c8825b72c5d92
Autor:
De Souza R. A., Alves F. R., De Oliveira C. M. G., Rosa J. M. O., De Assis Pinheiro J., De Aguiar G. P., Moraes W. B.
Publikováno v:
Helminthologia, Vol 58, Iss 2, Pp 213-216 (2021)
Samples of black pepper root with the presence of galls from the most southern region of the State of Bahia, Brazil, were characterized biochemically and morphologically using three criteria: i) observation of the anterior region of the males; ii) an
Externí odkaz:
https://doaj.org/article/a12742468f974f35b92eefc393c033ff
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:
Piscitelli, F., Moradi, F. Ghazi, Alves, F. S., Christensen, M. J., Hrivnak, J., Johansson, A., Fissum, K., Lai, C. C., Martinez, A. Monera, Pfeiffer, D., Shahu, E., Stahn, J., Svensson, P. O.
Publikováno v:
2024 JINST 19 P05010
The Multi-Blade (MB) Boron-10-based neutron detector is the chosen technology for three instruments at the European Spallation Source (ESS): the two ESS reflectometers, ESTIA and FREIA, and the Test Beam Line. A fourth MB detector has been built, ins
Externí odkaz:
http://arxiv.org/abs/2402.08325
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:
Lattanzi, V., Alves, F. O., Padovani, M., Fontani, F., Caselli, P., Ceccarelli, C., López-Sepulcre, A., Favre, C., Neri, R., Chahine, L., Vastel, C., Evans, L.
Publikováno v:
A&A 671, A35 (2023)
The study of the early phases of star and planet formation is important to understand the physical and chemical history of stellar systems such as our own. In particular, protostars born in rich clusters are prototypes of the young Solar System. In t
Externí odkaz:
http://arxiv.org/abs/2301.10267
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:
Asensio, J. Ferrer, Spezzano, S., Caselli, P., Alves, F. O., Sipilä, O., Redaelli, E., Bizzocchi, L., Lique, F., Mullins, A.
Spectral line profiles of several molecules observed towards the pre-stellar core L1544 appear double-peaked. For abundant molecular species this line morphology has been linked to self-absorption. However, the physical process behind the double-peak
Externí odkaz:
http://arxiv.org/abs/2209.02489
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