Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Aikutalp, A."'
Autor:
Kama, M., Bruderer, S., Carney, M., Hogerheijde, M., van Dishoeck, E. F., Fedele, D., Baryshev, A., Boland, W., Güsten, R., Aikutalp, A., Choi, Y., Endo, A., Frieswijk, W., Karska, A., Klaassen, P., Koumpia, E., Kristensen, L., Leurini, S., Nagy, Z., Beaupuits, J. -P. Perez, Risacher, C., van der Marel, N., van Kempen, T. A., van Weeren, R. J., Wyrowski, F., Yıldız, U. A.
Publikováno v:
A&A 588, A108 (2016)
The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming in them. The key gas-phase carbon carriers CO, C$^{0}$ and C$^{+}$ can now be observed in disks. The gas-phase ca
Externí odkaz:
http://arxiv.org/abs/1601.01449
Autor:
Kama, M., Bruderer, S., Carney, M., Hogerheijde, M., van Dishoeck, E. F., Fedele, D., Baryshev, A., Boland, W., Gusten, R., Aikutalp, A., Choi, Y., Endo, A., Frieswijk, W., Karska, A., Klaassen, P., Koumpia, E., Kristensen, L., Leurini, S., Nagy, Z., Perez Beaupuits, J.-P., Risacher, C., van der Marel, N., van Kempen, T. A., van Weeren, R. J., Wyrowski, F., Yildiz, U. A.
Publikováno v:
VizieR Online Data Catalog, 358. VizieR
APEX CHAMP+ and FLASH spectra of CI 1-0, CI 2-1, and CO 6-5 towards protoplanetary disks. The data was delivered from the telescope in reduced form and is on the Ta (K) scale. Baselines have been subtracted with low-order (order 0,1,2) polynomials. O
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=narcis______::31d4eb10b33ca397f78469768f803bc3
https://research.rug.nl/en/publications/368359ba-1234-47e2-8704-217f799040ca
https://research.rug.nl/en/publications/368359ba-1234-47e2-8704-217f799040ca
Autor:
Z. Nagy, A. Aikutalp, J. P. Perez Beaupuits, Akira Endo, E. F. van Dishoeck, R. Güsten, Christophe Risacher, E. Koumpia, N. van der Marel, P. D. Klaassen, Agata Karska, M. Kama, Andrey M. Baryshev, Umut A. Yildiz, Davide Fedele, Friedrich Wyrowski, Lars E. Kristensen, R. J. van Weeren, S. Leurini, W. Boland, Michiel R. Hogerheijde, T. A. van Kempen, Yun-Young Choi, M. T. Carney, S. Bruderer, W. Frieswijk
Publikováno v:
Astronomy and Astrophysics, 588, A108
Astronomy and astrophysics, 588:A108. EDP Sciences
Astronomy and astrophysics, 588:A108. EDP Sciences
Context. The gas-solid budget of carbon in protoplanetary disks is related to the composition of the cores and atmospheres of the planets forming in them. The principal gas-phase carbon carriers CO, C0, and C+ can now be observed regularly in disks.