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Cited article:
I. Hunter, P. L. Dufton, R. S. I. Ryans, D. J. Lennon, W. R. J. Rolleston, I. Hubeny, T. Lanz
A&A, 436 2 (2005) 687-695
Published online: 2005-05-30
This article has been cited by the following article(s):
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A Be star with a low nitrogen abundance in the
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The iron abundance of the Magellanic Bridge
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The VLT-FLAMES survey of massive stars: surface chemical
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THERMAL PRESSURES IN THE INTERSTELLAR MEDIUM OF THE MAGELLANIC CLOUDS
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Atmospheric parameters and rotational velocities for a sample of Galactic B-type supergiants
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A non-LTE abundance analysis of the post-AGB star ROA 5701
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Interstellar Gas-phase Element Depletions in the Small Magellanic Cloud: A Guide to Correcting for Dust in QSO Absorption Line Systems
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Discovery of O stars in the tidal Magellanic Bridge
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Testing the effects of opacity and the chemical mixture on the excitation of pulsations in B stars of the Magellanic Clouds
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Monthly Notices of the Royal Astronomical Society 422 (4) 3460 (2012)
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Chemical Composition of Two HiiRegions in NGC 6822 Based on VLT Spectroscopy
Antonio Peimbert, Manuel Peimbert and Maria Teresa Ruiz
The Astrophysical Journal 634 (2) 1056 (2005)
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ANALYSIS OF TWO SMALL MAGELLANIC CLOUD H II REGIONS CONSIDERING THERMAL INHOMOGENEITIES: IMPLICATIONS FOR THE DETERMINATIONS OF EXTRAGALACTIC CHEMICAL ABUNDANCES
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The Astrophysical Journal 746 (2) 115 (2012)
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Iron abundances from optical Fe iii absorption lines in B-type stellar spectra
H. M. A. Thompson, F. P. Keenan, P. L. Dufton, C. Trundle, R. S. I. Ryans and P. A. Crowther
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VLT UVES Observations of Interstellar Molecules and Diffuse Bands in the Magellanic Clouds
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C
ii
Abundances in Early-Type Stars: Solution to a Notorious Non-LTE Problem
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The Astrophysical Journal 639 (1) L39 (2006)
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Chemical Composition of B-type Stars from LAMOST DR5
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The Astrophysical Journal 937 (2) 110 (2022)
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Origins of B-type stars at high Galactic latitudes based on abundances and kinematics
Zhicun Liu, Wenyuan Cui, Gang Zhao, Chao Liu, Changqing Luo and Sofya Alexeeva
Monthly Notices of the Royal Astronomical Society 519 (1) 995 (2022)
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