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pro vyhledávání: '"Gusdorf, A"'
Autor:
Tornero, Angélica1,2 angelica.tornero.s@gmail.com
Publikováno v:
Káñina. Revista de Artes y Letras de la Universidad de Costa Rica. ene-abr2023, Vol. 47 Issue 1, p71-93. 23p.
Autor:
Angélica Tornero
Publikováno v:
Metáfora, Vol 4, Iss 7 (2021)
Desde el último tercio del siglo xx, observamos la propagación de escrituras en las que el yo autoral está implicado de distintas maneras. Paralelamente, se ha incrementado el interés de teóricos y críticos por examinar el fenómeno. En términ
Externí odkaz:
https://doaj.org/article/0cbace89939744a2b9562e9c6bbb2fc5
Autor:
Angélica Tornero
Publikováno v:
Káñina, Vol 47, Iss 1 (2023)
Los estudios de las escrituras autobiográficas han aumentado notablemente desde la segunda mitad del siglo XX. Teóricos y críticos de diversas disciplinas, como la filosofía, la literatura, la psicología, la historia, la antropología y la educa
Externí odkaz:
https://doaj.org/article/6bd8a7dce4294a61bd9991fa6dae752f
Autor:
Reach, William T., Tram, Ngoc Le, DeWitt, Curtis, Lesaffre, Pierre, Godard, Benjamin, Gusdorf, Antoine
Supernova shocks into dense molecular cores in IC 443 (clumps B, C, and G) and 3C 391 were observed using the Stratospheric Observatory for Infrared Astronomy and complemented by archival data from the Herschel Space Observatory. The pure rotational
Externí odkaz:
http://arxiv.org/abs/2410.22580
Autor:
Gouellec, Valentin J. M. Le, Lew, Ben W. P., Greene, Thomas P., Johnstone, Doug, Gusdorf, Antoine, Francis, Logan, DeWitt, Curtis, Meyer, Michael, Tychoniec, Łukasz, van Dishoeck, Ewine F., Barsony, Mary, Hodapp, Klaus W., Robberto, Massimo
The near-infrared (NIR) emission of the youngest protostars still needs to be characterized to better understand the evolution of their accretion and ejection activity. We analyze James Webb Space Telescope NIRSpec 1.7 -- 5.3 $\mu$m observations of t
Externí odkaz:
http://arxiv.org/abs/2410.11095
Autor:
Sandoval-Garrido, N. A., Stutz, A. M., Álvarez-Gutiérrez, R. H., Galván-Madrid, R., Motte, F., Ginsburg, A., Cunningham, N., Reyes-Reyes, S., Redaelli, E., Bonfand, M., Salinas, J., Koley, A., Braine, J., Bronfman, L., Busquet, G., Csengeri, T., Di Francesco, J., Fernández-López, M., Garcia, P., Gusdorf, A., Liu, H. -L., Sanhueza, P.
ALMA-IMF observed 15 massive protoclusters capturing multiple spectral lines and the continuum emission. We focus on the G351.77 protocluster ($\sim$ 2500 M$_{\odot}$, estimated from single-dish continuum observations) located at 2 kpc. We trace the
Externí odkaz:
http://arxiv.org/abs/2410.09843
Autor:
Neufeld, David A., DeWitt, Curtis, Lesaffre, Pierre, Cabrit, Sylvie, Gusdorf, Antoine, Tram, Le Ngoc, Reach, William T.
Using the EXES instrument on SOFIA, we have obtained velocity-resolved spectra of several pure rotational lines of H2 toward shocked molecular gas within three Galactic sources: the supernova remnant (SNR) IC443 (Clump C), a protostellar outflow in t
Externí odkaz:
http://arxiv.org/abs/2410.04473
Akademický článek
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Publikováno v:
A&A 690, L18 (2024)
Abridged: We present the first observation of the HCO+(1-0) and HCN(1-0) emission in the northern filaments of Centaurus A with ALMA. HCO+(1-0) is detected in 9 clumps of the Horseshoe complex, with similar velocities as the CO(1-0) emission. Convers
Externí odkaz:
http://arxiv.org/abs/2409.11031
Autor:
Louvet, F., Sanhueza, P., Stutz, A., Men'shchikov, A., Motte, F., Galván-Madrid, R., Bontemps, S., Pouteau, Y., Ginsburg, A., Csengeri, T., Di Francesco, J., Dell'Ova, P., González, M., Didelon, P., Braine, J., Cunningham, N., Thomasson, B., Lesaffre, P., Hennebelle, P., Bonfand, M., Gusdorf, A., Álverez-Gutiérrez, R. H., Nony, T., Busquet, G., Olguin, F., Bronfman, L., Salinas, J., Fernandez-Lopez, M., Moraux, E., Liu, H. L., Lu, X., Huei-Ru, V., Towner, A., Valeille-Manet, M., Brouillet, N., Herpin, F., Lefloch, B., Baug, T., Maud, L., Lopez-Sepulcre, A., Svodoba, B.
Publikováno v:
A&A 690, A33 (2024)
The stellar initial mass function (IMF) is critical to our understanding of star formation and the effects of young stars on their environment. On large scales, it enables us to use tracers such as UV or Halpha emission to estimate the star formation
Externí odkaz:
http://arxiv.org/abs/2407.18719