Orbital evolution of planetesimals in gaseous disks
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DOI[10.1186/s40623-015-0218-y]to the data of the same series
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Bibliographic Record
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- Material Type
- 記事
- Author/Editor
- Hiroshi Kobayashi
- Publication, Distribution, etc.
- Publication Date
- 2015-04-30
- Publication Date (W3CDTF)
- 2015-04-30
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 67(60)
- Volume
- 67(60)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-015-0218-y
- Persistent ID (NDL)
- info:ndljp/pid/9483545
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2015-08-17T20:47:01+09:00
- Date Captured (W3CDTF)
- 2015-06-20
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/9227920
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- コレクション : 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- DOI
- 10.1186/s40623-015-0218-y10.48550/arxiv.1505.01568
- Access Restrictions
- インターネット公開
- Related Material (URI)
- Is Referenced By
- Distribution of Captured Planetesimals in Circumplanetary Gas Disks and Implications for Accretion of Regular SatellitesFrom Planetesimal to Planet in Turbulent Disks. II. Formation of Gas Giant PlanetsFROM PLANETESIMALS TO PLANETS IN TURBULENT PROTOPLANETARY DISKS. I. ONSET OF RUNAWAY GROWTHCollisional elongation: Possible origin of extremely elongated shape of 1I/‘OumuamuaRapid Formation of Gas-giant Planets via Collisional Coagulation from Dust Grains to Planetary Cores
- References
- ON THE VIABILITY OF THE MAGNETOROTATIONAL INSTABILITY IN CIRCUMPLANETARY DISKSTEMPORARY CAPTURE OF PLANETESIMALS BY A PLANET FROM THEIR HELIOCENTRIC ORBITSPlanetary growth with collisional fragmentation and gas dragTemporary capture of planetesimals by a giant planet and implication for the origin of irregular satellitesNebular Gas Drag and Planetary AccretionCAPTURE OF PLANETESIMALS BY GAS DRAG FROM CIRCUMPLANETARY DISKSPLANETARY CORE FORMATION WITH COLLISIONAL FRAGMENTATION AND ATMOSPHERE TO FORM GAS GIANT PLANETSThree‐dimensional Interaction between a Planet and an Isothermal Gaseous Disk. I. Corotation and Lindblad Torques and Planet MigrationThe evidence of an early stellar encounter in Edgeworth–Kuiper beltThe Gas Drag Effect on the Elliptic Motion of a Solid Body in the Primordial Solar Nebula
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 雑誌記事索引データベースCrossref科学研究費助成事業データベースCrossrefCrossrefCrossrefCrossrefCrossref
- Bibliographic ID (NDL)
- 9483545