Zobrazeno 1 - 10
of 1 313
pro vyhledávání: '"Larsson, B A"'
Autor:
Kamp, I., Honda, M., Nomura, H., Audard, M., Fedele, D., Waters, L. B. F. M., Aikawa, Y., Banzatti, A., Bowey, J. E., Bradford, M., Dominik, C., Furuya, K., Habart, E., Ishihara, D., Johnstone, D., Kennedy, G., Kim, M., Kral, Q., Lai, S. P., Larsson, B., McClure, M., Miotello, A., Momose, M., Nakagawa, T., Naylor, D., Nisini, B., Notsu, S., Onaka, T., Pantin, E., Podio, L., Marichalar, P. Riviere, Rocha, W. R. M., Roelfsema, P., Santos, F., Shimonishi, T., Tang, Y. W., Takami, M., Tazaki, R., Wolf, S., Wyatt, M., Ysard, N.
In this era of spatially resolved observations of planet forming disks with ALMA and large ground-based telescopes such as the VLT, Keck and Subaru, we still lack statistically relevant information on the quantity and composition of the material that
Externí odkaz:
http://arxiv.org/abs/2106.13782
Publikováno v:
A&A 647, A86 (2021)
The Odin satellite is now into its twentieth year of operation, much surpassing its design life of two years. One of its major pursuits was the search for and study of H2O in the Solar System and the Milky Way galaxy. Herschel has observed the centra
Externí odkaz:
http://arxiv.org/abs/2101.03876
Publikováno v:
A&A 628, A127 (2019)
The debris disk surrounding $\beta$~Pictoris has been observed with ALMA to contain a belt of CO gas with a distinct peak at $\sim$85 au. This CO clump is thought to be the result of a region of enhanced density of solids that collide and release CO
Externí odkaz:
http://arxiv.org/abs/1906.11106
Autor:
Roelfsema, P. R., Shibai, H., Armus, L., Arrazola, D., Audard, M., Audley, M. D., Bradford, C. M., Charles, I., Dieleman, P., Doi, Y., Duband, L., Eggens, M., Evers, J., Funaki, I., Gao, J. R., Giard, M., Fernández, A. di Giorgio L. M. González, Griffin, M., Helmich, F. P., Hijmering, R., Huisman, R., Ishihara, D., Isobe, N., Jackson, B., Jacobs, H., Jellema, W., Kamp, I., Kaneda, H., Kawada, M., Kemper, F., Kerschbaum, F., Khosropanah, P., Kohno, K., Kooijman, P. P., Krause, O., van der Kuur, J., Kwon, J., Laauwen, W. M., de Lange, G., Larsson, B., van Loon, D., Madden, S. C., Matsuhara, H., Najarro, F., Nakagawa, T., Naylor, D., Ogawa, H., Onaka, T., Oyabu, S., Poglitsch, A., Reveret, V., Rodriguez, L., Spinoglio, L., Sakon, I., Sato, Y., Shinozaki, K., Shipman, R., Sugita, H., Suzuki, T., van der Tak, F. F. S., Redondo, J. Torres, Wada, T., Wang, S. Y., Wafelbakker, C. K., van Weers, H., Withington, S., Vandenbussche, B., Yamada, T., Yamamura, I.
Measurements in the infrared wavelength domain allow us to assess directly the physical state and energy balance of cool matter in space, thus enabling the detailed study of the various processes that govern the formation and early evolution of stars
Externí odkaz:
http://arxiv.org/abs/1803.10438
Autor:
Staaf Larsson, B.1,2 (AUTHOR) Birgitta.Staaf.Larsson@slu.se, Dahlborn, K.1 (AUTHOR), Jansson, A.1 (AUTHOR)
Publikováno v:
Acta Agriculturae Scandinavica: Section A, Animal Science. Dec2024, p1-8. 8p. 2 Illustrations, 3 Charts.
Autor:
Sandqvist, Aa., Larsson, B., Hjalmarson, Å., Encrenaz, P., Gerin, M., Goldsmith, P. F., Lis, D. C., Liseau, R., Pagani, L., Roueff, E., Viti, S.
Publikováno v:
A&A 584, A118 (2015)
To date O2 has definitely been detected in only two sources, namely rho Oph A and Orion, reflecting the extremely low abundance of O2 in the interstellar medium. One of the sources in the HOP program is the +50 km/s Cloud in the Sgr A Complex in the
Externí odkaz:
http://arxiv.org/abs/1510.06620
Autor:
Liseau, R., Larsson, B., Lunttila, T., Olberg, M., Rydbeck, G., Bergman, P., Justtanont, K., Olofsson, G., de Vries, B. L.
We aim at determining the spatial distribution of the gas and dust in star-forming regions and address their relative abundances in quantitative terms. We also examine the dust opacity exponent beta for spatial and/or temporal variations. Using mappi
Externí odkaz:
http://arxiv.org/abs/1504.06277
Autor:
Staaf Larsson, B., Jansson, A., Holmberg, M., Winblad von Walter, L., Stéen, M., Dahlborn, K.
Publikováno v:
Acta Agriculturae Scandinavica: Section A, Animal Science; Sep-Dec2024, Vol. 73 Issue 3/4, p153-164, 12p
Akademický článek
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Autor:
Bjerkeli, P., Liseau, R., Brinch, C., Olofsson, G., Santangelo, G., Cabrit, S., Benedettini, M., Black, J. H., Herczeg, G., Justtanont, K., Kristensen, L. E., Larsson, B., Nisini, B., Tafalla, M.
Publikováno v:
A&A 571, A90 (2014)
The HH54 shock is a Herbig-Haro object, located in the nearby Chamaeleon II cloud. Observed CO line profiles are due to a complex distribution in density, temperature, velocity, and geometry. Resolving the HH54 shock wave in the far-infrared cooling
Externí odkaz:
http://arxiv.org/abs/1409.8111