Zobrazeno 1 - 10
of 16
pro vyhledávání: '"Tanner, J. D."'
Main sequence, solar-like stars (M < 1.5 Msun) have outer convective envelopes that are sufficiently thick to affect significantly their overall structure. The radii of these stars, in particular, are sensitive to the details of inefficient, super-ad
Externí odkaz:
http://arxiv.org/abs/1811.01817
Publikováno v:
Astron.Astrophys. 461 (2007) 767-773
The stellar abundance ratio of Mg/Fe is an important tool in diagnostics of galaxy evolution. In order to make reliable measurements of the Mg abundance of stars, it is necessary to have accurate values for the oscillator strength (f-value) of each o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0610033
Autor:
Norton, A. J., Tanner, J. D.
We present the first optical photometry of the counterpart to the candidate intermediate polar RX J0153.3+7446. This reveals an optical pulse period of 2333s +/- 5s. Reanalysis of the previously published ROSAT X-ray data reveals that the true X-ray
Externí odkaz:
http://arxiv.org/abs/astro-ph/0512145
Publikováno v:
Scopus-Elsevier
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::842e9c0bac21fd96a9c4a31781a76204
http://cds.cern.ch/record/1099551
http://cds.cern.ch/record/1099551
Akademický článek
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Autor:
Aldenius, M., Tanner, J. D., Johansson, S., Lundberg, H., Ryan, S. G., Aldenius, M., Tanner, J. D., Johansson, S., Lundberg, H., Ryan, S. G.
Publikováno v:
Astronomy and Astrophysics; January 2007, Vol. 461 Issue: 2 p767-773, 7p
