Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Ag��ndez, M."'
Autor:
Fonfr��a, J. P., Montiel, E. J., Cernicharo, J., DeWitt, C. N., Richter, M. J., Lacy, J. H., Greathouse, T. K., Santander-Garc��a, M., Ag��ndez, M., Massalkhi, S.
High spectral resolution observations toward the low mass-loss rate C-rich, J-type AGB star Y CVn have been carried out at 7.5, 13.1 and 14.0 um with SOFIA/EXES and IRTF/TEXES. Around 130 HCN and H13CN lines of bands v2, 2v2, 2v2-v2, 3v2-2v2, 3v2-v2,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d94221254dae88cb9c7780863617dfa7
http://arxiv.org/abs/2105.01411
http://arxiv.org/abs/2105.01411
Autor:
Velilla-Prieto, L., Cernicharo, J., Ag��ndez, M., Fonfr��a, J. P., Quintana-Lacaci, G., Marcelino, N., Castro-Carrizo, A.
The study of the gas in the envelopes surrounding asymptotic giant branch (AGB) stars through observations in the millimetre wavelength range provides information about the history and nature of these molecular factories. Here we present ALMA observa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::762743936fb919bb249386b77bd3dca0
Autor:
De Beck, E., Lombaert, R., Ag��ndez, M., Daniel, F., Decin, L., Cernicharo, J., M��ller, H. S. P., Min, M., Royer, P., Vandenbussche, B., de Koter, A., Waters, L. B. F. M., Groenewegen, M. A. T., Barlow, M. J., Gu��lin, M., Kahane, C., Pearson, J. C., Encrenaz, P., Szczerba, R., Schmidt, M. R.
The C-rich AGB star IRC+10216 undergoes strong mass loss, and quasi-periodic density enhancements in the circumstellar matter have been reported. CO is ubiquitous in the CSE, while CCH emission comes from a spatially confined shell. With the IRAM 30m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1b057b68aa017d4b549f0255ac0967a6
http://arxiv.org/abs/1201.1850
http://arxiv.org/abs/1201.1850
Autor:
Decin, L., Cernicharo, J., Barlow, M. J., Royer, P., Vandenbussche, B., Wesson, R., Polehampton, E. T., De Beck, E., Ag��ndez, M., Blommaert, J. A. D. L., Cohen, M., Daniel, F., De Meester, W., Exter, K., Feuchtgruber, H., Fonfria, J. P., Gear, W. K., Goicoechea, J. R., Gomez, H. L., Groenewegen, M. A. T., Hargrave, P. C., Huygen, R., Imhof, P., Ivison, R. J., Jean, C., Kerschbaum, F., Leeks, S. J., Lim, T., Matsuura, M., Olofsson, G., Posch, T., Regibo, S., Savini, G., Sibthorpe, B., Swinyard, B. M., Tercero, B., Waelkens, C., Witherick, D. K., Yates, J. A.
The interstellar medium is enriched primarily by matter ejected from evolved low and intermediate mass stars. The outflows from these stars create a circumstellar envelope in which a rich gas-phase and dust-nucleation chemistry takes place. We observ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7538a35c92c542f4d7ee0773316c134d
http://arxiv.org/abs/1005.4675
http://arxiv.org/abs/1005.4675
Publikováno v:
Astronomy and Astrophysics; March 2010, Vol. 479 Issue: 2 p493-501, 9p
Publikováno v:
Astronomy and Astrophysics; January 2008, Vol. 478 Issue: 1 pL19-L22, 4p