Zobrazeno 1 - 10
of 16
pro vyhledávání: '"GARMANY, C. D."'
Autor:
Braganca, G. A., Daflon, S., Lanz, T., Cunha, K., Bensby, T., McMillan, P. J., Garmany, C. D., Glaspey, J. W., Fernandes, M. Borges, Oey, M. S., Hubeny, I.
Publikováno v:
A&A 625, A120 (2019)
Using a sample of 31 main-sequence OB stars located between galactocentric distances 8.4 - 15.6 kpc, we aim to probe the present-day radial abundance gradients of the Galactic disk. The analysis is based on high-resolution spectra obtained with the M
Externí odkaz:
http://arxiv.org/abs/1904.04340
Autor:
Bragança, G. A., Lanz, T., Daflon, S., Cunha, K., Garmany, C. D., Glaspey, J. W., Fernandes, M. Borges, Oey, M. S., Bensby, T., Hubeny, I.
The aim of this study is to analyse and determine elemental abundances for a large sample of distant B stars in the outer Galactic disk in order to constrain the chemical distribution of the Galactic disk and models of chemical evolution of the Galax
Externí odkaz:
http://arxiv.org/abs/1408.5807
Publikováno v:
Publications of the Astronomical Society of the Pacific, 1986 Jan 01. 98(599), 29-29.
Externí odkaz:
https://www.jstor.org/stable/40678626
Akademický článek
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Autor:
Driel-Gesztelyi, L., Meynet, G., Gaizauskas, V., Cook, J. W., McKenna-Lawlor, S. M. P., Garmany, C. D., Jugaku, Jun, Lamers, Henny J. G. L. M., Achterberg, A., Greve, J. P., Dommanget, J., Kruit, P. C.
Publikováno v:
Space Science Reviews; March 1993, Vol. 64 Issue: 1-2 p165-174, 10p
Autor:
Garmany, C. D.
Publikováno v:
Publications of the Astronomical Society of the Pacific; October 1984, Vol. 96 Issue: 584 p779-782, 4p
Autor:
Marov, M. Ya, Garmany, C. D., Heck, André, Schadee, A., McNally, D., Kruit, P. C., Pecker, J.-C., Jager, Cornelis, Somov, B. V.
Publikováno v:
Space Science Reviews; April 1989, Vol. 49 Issue: 3-4 p385-390, 6p
Autor:
Garmany, C. D., Massey, P.
Publikováno v:
Publications of the Astronomical Society of the Pacific; August 1981, Vol. 93 Issue: 554 p500-503, 4p
Publikováno v:
NASA Astrophysics Data System
The WN 5 star HD 50896 has been the subject of many variability studies in the optical. A period of 3.766 days is frequently associated with this variability although it is by no means clear whether it reflects, for example, binary motions or rotatio
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::afe6d6e7b95d70eaeda02a3252b52c29
https://ui.adsabs.harvard.edu/#abs/1991IAUS..143..179S
https://ui.adsabs.harvard.edu/#abs/1991IAUS..143..179S
Autor:
Bragançca, G. A., Lanz, T., Daflon, S., Cunha, K., Garmany, C. D., Glaspey, J. W., Borges Fernandes, M., Oey, M. S., Bensby, T., Hubeny, I., Meynet, Georges, Georgy, Cyril, Groh, José, Stee, Philippe
Publikováno v:
Proceedings of the International Astronomical Union; Jun2014 Supplement, Vol. 9 Issue S307, p90-91, 2p