Line formation in convective stellar atmospheres - I. Granulation corrections for solar photospheric abundances

被引：0

作者：

Steffen, M. ^{[1
]}

Holweger, H. ^{[1
]}

机构：

[1] Astrophysikalisches Institut Potsdam, An der Sternwarte 16, 14482 Potsdam, Germany

来源：

| 1600年 / EDP Sciences卷 / 387期

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共 50 条

[1] Line formation in convective stellar atmospheres - I. Granulation corrections for solar photospheric abundances
Steffen, M
Holweger, H
ASTRONOMY & ASTROPHYSICS, 2002, 387 (01) : 258 - 270
[2] Line formation in solar granulation III. The photospheric Si and meteoritic Fe abundances
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[3] Solar and stellar photospheric abundances
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[4] Solar and stellar photospheric abundances
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[5] Photospheric metal abundances in active stellar atmospheres
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[6] Balmer line formation in convective stellar atmospheres
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[7] On the line formation process in stellar atmospheres - I. Unpolarized light
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[8] STELLAR GRANULATION .2. STELLAR PHOTOSPHERIC LINE ASYMMETRIES
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[9] Line formation in solar granulation -: I.: Fe line shapes, shifts and asymmetries
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Prieto, CA
Stein, RF
ASTRONOMY & ASTROPHYSICS, 2000, 359 (02) : 729 - 742
[10] Line formation in solar granulation -: II.: The photospheric Fe abundance
Asplund, M
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Trampedach, R
Stein, RF
ASTRONOMY & ASTROPHYSICS, 2000, 359 (02) : 743 - 754

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