UV and optical quantitative spectroscopy of early B-type supergiants in M 33
2003 ◽
Vol 212
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pp. 249-250
Keyword(s):
The One
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We present the analysis of UV and optical spectra of M 33 early B-type supergiants. Stellar parameters, metal abundances (Si, Mg, O and N) and mass loss rates are derived from anlyses of optical spectra by means of non-LTE unblanketed unified model atmospheres (fastwind code, Santolaya-Rey, Puls & Herrero 1997). These analyses use wind terminal velocities previously derived from the analysis of UV P-Cygni profiles. Stellar radial gradients of Si, O and Mg are derived for the M 33 disk. Differential abundances of those elements with respect to Galactic counterparts are also presented, along with nitrogen. Finally, the wind momenta of M 33 stars is derived and compared with the one found for Galactic B-type supergiants.
2020 ◽
Vol 499
(2)
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pp. 1531-1560
Keyword(s):
Keyword(s):
1979 ◽
Vol 83
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pp. 431-445
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Keyword(s):
2019 ◽
Vol 623
◽
pp. A119
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Keyword(s):
1987 ◽
Vol 122
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pp. 227-228