Slow relative motion of IRAS galaxies at small separations: implications for galaxy formation models
Gespeichert in:
| Beteiligte Personen: | , , |
|---|---|
| Format: | Buch |
| Sprache: | Englisch |
| Veröffentlicht: |
Garching
MPA
2002
|
| Umfang: | 4 S. graph. Darst. : 30 cm |
Internformat
MARC
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| 100 | 1 | |a Jing, Yipeng |e Verfasser |4 aut | |
| 245 | 1 | 0 | |a Slow relative motion of IRAS galaxies at small separations |b implications for galaxy formation models |c Y. P. Jing, G. Börner, and Y. Suto. Partner Group of the MPA at Shanghai Observatory ; [Max-Planck-Institut für Astrophysik, Garching] |
| 264 | 1 | |a Garching |b MPA |c 2002 | |
| 300 | |a 4 S. |b graph. Darst. : 30 cm | ||
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| 700 | 1 | |a Börner, Gerhard |d 1941- |e Verfasser |0 (DE-588)129450316 |4 aut | |
| 700 | 1 | |a Sutō, Yasushi |e Verfasser |4 aut | |
| 943 | 1 | |a oai:aleph.bib-bvb.de:BVB01-009898682 | |
Datensatz im Suchindex
| _version_ | 1818957130228563968 |
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| any_adam_object | |
| author | Jing, Yipeng Börner, Gerhard 1941- Sutō, Yasushi |
| author_GND | (DE-588)129450316 |
| author_facet | Jing, Yipeng Börner, Gerhard 1941- Sutō, Yasushi |
| author_role | aut aut aut |
| author_sort | Jing, Yipeng |
| author_variant | y j yj g b gb y s ys |
| building | Verbundindex |
| bvnumber | BV014557043 |
| ctrlnum | (OCoLC)76343906 (DE-599)BVBBV014557043 |
| format | Book |
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| id | DE-604.BV014557043 |
| illustrated | Illustrated |
| indexdate | 2024-12-20T11:04:57Z |
| institution | BVB |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-009898682 |
| oclc_num | 76343906 |
| open_access_boolean | |
| owner | DE-12 DE-19 DE-BY-UBM |
| owner_facet | DE-12 DE-19 DE-BY-UBM |
| physical | 4 S. graph. Darst. : 30 cm |
| publishDate | 2002 |
| publishDateSearch | 2002 |
| publishDateSort | 2002 |
| publisher | MPA |
| record_format | marc |
| spelling | Jing, Yipeng Verfasser aut Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models Y. P. Jing, G. Börner, and Y. Suto. Partner Group of the MPA at Shanghai Observatory ; [Max-Planck-Institut für Astrophysik, Garching] Garching MPA 2002 4 S. graph. Darst. : 30 cm txt rdacontent n rdamedia nc rdacarrier Börner, Gerhard 1941- Verfasser (DE-588)129450316 aut Sutō, Yasushi Verfasser aut |
| spellingShingle | Jing, Yipeng Börner, Gerhard 1941- Sutō, Yasushi Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models |
| title | Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models |
| title_auth | Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models |
| title_exact_search | Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models |
| title_full | Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models Y. P. Jing, G. Börner, and Y. Suto. Partner Group of the MPA at Shanghai Observatory ; [Max-Planck-Institut für Astrophysik, Garching] |
| title_fullStr | Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models Y. P. Jing, G. Börner, and Y. Suto. Partner Group of the MPA at Shanghai Observatory ; [Max-Planck-Institut für Astrophysik, Garching] |
| title_full_unstemmed | Slow relative motion of IRAS galaxies at small separations implications for galaxy formation models Y. P. Jing, G. Börner, and Y. Suto. Partner Group of the MPA at Shanghai Observatory ; [Max-Planck-Institut für Astrophysik, Garching] |
| title_short | Slow relative motion of IRAS galaxies at small separations |
| title_sort | slow relative motion of iras galaxies at small separations implications for galaxy formation models |
| title_sub | implications for galaxy formation models |
| work_keys_str_mv | AT jingyipeng slowrelativemotionofirasgalaxiesatsmallseparationsimplicationsforgalaxyformationmodels AT bornergerhard slowrelativemotionofirasgalaxiesatsmallseparationsimplicationsforgalaxyformationmodels AT sutoyasushi slowrelativemotionofirasgalaxiesatsmallseparationsimplicationsforgalaxyformationmodels |