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Carbon and M-type giant stars in the Magellanic Clouds
B.M. Blanco
(
Cerro-Tololo InterAmerican Obs.
)
,
V.M. Blanco
(
Cerro-Tololo InterAmerican Obs.
)
,
M.F. McCarthy
(
Vatican Astron. Observ.
)
Feb, 1978
2 pages
Published in:
Nature
271
(1978)
638-639
DOI:
10.1038/271638a0
View in:
ADS Abstract Service
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17 citations
Citations per year
1986
1993
2000
2007
2013
1
0
2
3
References
(14)
Figures
(0)
Astrophys.J.
109
391
edit
Publ.Astron.Soc.Pac.
85
174
edit
Publ.Astron.Soc.Pac.
88
860
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Astron.J.
62
205
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Magellanic clouds
B.J. Bok
Ann.Rev.Astron.Astrophys.
4
(1966)
95-144
•
DOI:
10.1146/annurev.aa.04.090166.000523
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Nature
258
407
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Astrophys.J.Suppl.
2
1
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Mon.Not.Roy.Astron.Soc.
164
15P
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The Physical properties of carbon stars
George Wallerstein
(
Washington U., Seattle, Astron. Dept.
)
Ann.Rev.Astron.Astrophys.
11
(1973)
115-134
•
DOI:
10.1146/annurev.aa.11.090173.000555
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Astrophys.J.
153
915
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Publ.Astron.Soc.Pac.
80
597
edit
IAU Symp.
20
239
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Astrophys.J.
203
L81
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Bull.Am.Astron.Soc.
8
537
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