Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants?:
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Format: | Buch |
| Sprache: | German |
| Veröffentlicht: |
Garching bei München
Max-Planck-Inst. für Astrophysik
1996
|
| Schriftenreihe: | Max-Planck-Institut für Astrophysik <Garching, München>: MPA
941 |
| Beschreibung: | 12 S. graph. Darst. |
Internformat
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| 100 | 1 | |a Denisenkov, Pavel A. |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? |c P. A. Denissenkov, J. Wagenhuber and Achim Weiss. Max-Planck-Institut für Astrophysik |
| 264 | 1 | |a Garching bei München |b Max-Planck-Inst. für Astrophysik |c 1996 | |
| 300 | |a 12 S. |b graph. Darst. | ||
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| 338 | |b nc |2 rdacarrier | ||
| 490 | 1 | |a Max-Planck-Institut für Astrophysik <Garching, München>: MPA |v 941 | |
| 700 | 1 | |a Wagenhuber, Josef |e Verfasser |4 aut | |
| 700 | 1 | |a Weiss, Achim |e Verfasser |4 aut | |
| 830 | 0 | |a Max-Planck-Institut für Astrophysik <Garching, München>: MPA |v 941 |w (DE-604)BV009868828 |9 941 | |
| 999 | |a oai:aleph.bib-bvb.de:BVB01-007256016 | ||
Datensatz im Suchindex
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| author | Denisenkov, Pavel A. Wagenhuber, Josef Weiss, Achim |
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| bvnumber | BV010854807 |
| ctrlnum | (OCoLC)75744640 (DE-599)BVBBV010854807 |
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| id | DE-604.BV010854807 |
| illustrated | Illustrated |
| indexdate | 2024-07-09T18:00:02Z |
| institution | BVB |
| language | German |
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| publishDate | 1996 |
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| publisher | Max-Planck-Inst. für Astrophysik |
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| series | Max-Planck-Institut für Astrophysik <Garching, München>: MPA |
| series2 | Max-Planck-Institut für Astrophysik <Garching, München>: MPA |
| spelling | Denisenkov, Pavel A. Verfasser aut Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? P. A. Denissenkov, J. Wagenhuber and Achim Weiss. Max-Planck-Institut für Astrophysik Garching bei München Max-Planck-Inst. für Astrophysik 1996 12 S. graph. Darst. txt rdacontent n rdamedia nc rdacarrier Max-Planck-Institut für Astrophysik <Garching, München>: MPA 941 Wagenhuber, Josef Verfasser aut Weiss, Achim Verfasser aut Max-Planck-Institut für Astrophysik <Garching, München>: MPA 941 (DE-604)BV009868828 941 |
| spellingShingle | Denisenkov, Pavel A. Wagenhuber, Josef Weiss, Achim Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? Max-Planck-Institut für Astrophysik <Garching, München>: MPA |
| title | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? |
| title_auth | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? |
| title_exact_search | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? |
| title_full | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? P. A. Denissenkov, J. Wagenhuber and Achim Weiss. Max-Planck-Institut für Astrophysik |
| title_fullStr | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? P. A. Denissenkov, J. Wagenhuber and Achim Weiss. Max-Planck-Institut für Astrophysik |
| title_full_unstemmed | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? P. A. Denissenkov, J. Wagenhuber and Achim Weiss. Max-Planck-Institut für Astrophysik |
| title_short | Could intermediate mass AGB stars produce star to star abundance variations in globular cluster red giants? |
| title_sort | could intermediate mass agb stars produce star to star abundance variations in globular cluster red giants |
| volume_link | (DE-604)BV009868828 |
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