Geometry of highly inclined protoplanetary disks
We present a geometric model for the modelling of spectral energy distribution of inclined protoplanetary disks. We investigate peculiarities in the geometry of nearly edge-on disks with an inner hole and a central object. In the investigation we consider two cases: that of geometrically thin disks...
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| Veröffentlicht in: | Advances in Astronomy and Space Physics |
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| Datum: | 2015 |
| Hauptverfasser: | , , |
| Format: | Artikel |
| Sprache: | English |
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Головна астрономічна обсерваторія НАН України
2015
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| Online Zugang: | https://nasplib.isofts.kiev.ua/handle/123456789/119823 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Zitieren: | Geometry of highly inclined protoplanetary disks / O.V. Zakhozhay, C. del Burgo, V.A. Zakhozhay // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 33-38. — Бібліогр.: 16 назв. — англ. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-119823 |
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Zakhozhay, O.V. del Burgo, C. Zakhozhay, V.A. 2017-06-09T21:00:46Z 2017-06-09T21:00:46Z 2015 Geometry of highly inclined protoplanetary disks / O.V. Zakhozhay, C. del Burgo, V.A. Zakhozhay // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 33-38. — Бібліогр.: 16 назв. — англ. 2227-1481 DOI: 10.17721/2227-1481.5.33-38 https://nasplib.isofts.kiev.ua/handle/123456789/119823 We present a geometric model for the modelling of spectral energy distribution of inclined protoplanetary disks. We investigate peculiarities in the geometry of nearly edge-on disks with an inner hole and a central object. In the investigation we consider two cases: that of geometrically thin disks (where the star is larger than the rim of the inner edge of the disk) and that of eometrically thick disks (when the star is smaller than the inner rim of the disk). Our model is appropriate for modelling substellar objects with primordial gas-rich disks, as activity (such as accretion or outflows) in such disks has low amplitude and can be ignored even when modelling early evolution stages. Furthermore, it can also be used to model any symmetric system with a disk and a spherical central body (star, brown dwarf or giant planet). We are grateful to Dr. Yann Boehler for comments and suggestions which substantially improved this paper. en Головна астрономічна обсерваторія НАН України Advances in Astronomy and Space Physics Geometry of highly inclined protoplanetary disks Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Geometry of highly inclined protoplanetary disks |
| spellingShingle |
Geometry of highly inclined protoplanetary disks Zakhozhay, O.V. del Burgo, C. Zakhozhay, V.A. |
| title_short |
Geometry of highly inclined protoplanetary disks |
| title_full |
Geometry of highly inclined protoplanetary disks |
| title_fullStr |
Geometry of highly inclined protoplanetary disks |
| title_full_unstemmed |
Geometry of highly inclined protoplanetary disks |
| title_sort |
geometry of highly inclined protoplanetary disks |
| author |
Zakhozhay, O.V. del Burgo, C. Zakhozhay, V.A. |
| author_facet |
Zakhozhay, O.V. del Burgo, C. Zakhozhay, V.A. |
| publishDate |
2015 |
| language |
English |
| container_title |
Advances in Astronomy and Space Physics |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| description |
We present a geometric model for the modelling of spectral energy distribution of inclined protoplanetary disks. We investigate peculiarities in the geometry of nearly edge-on disks with an inner hole and a central object. In the investigation we consider two cases: that of geometrically thin disks (where the star is larger than the rim of the inner edge of the disk) and that of eometrically thick disks (when the star is smaller than the inner rim of the disk). Our model is appropriate for modelling substellar objects with primordial gas-rich disks, as activity (such as accretion or outflows) in such disks has low amplitude and can be ignored even when modelling early evolution stages. Furthermore, it can also be used to model any symmetric system with a disk and a spherical central body (star, brown dwarf or giant planet).
|
| issn |
2227-1481 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/119823 |
| citation_txt |
Geometry of highly inclined protoplanetary disks / O.V. Zakhozhay, C. del Burgo, V.A. Zakhozhay // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 33-38. — Бібліогр.: 16 назв. — англ. |
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AT zakhozhayov geometryofhighlyinclinedprotoplanetarydisks AT delburgoc geometryofhighlyinclinedprotoplanetarydisks AT zakhozhayva geometryofhighlyinclinedprotoplanetarydisks |
| first_indexed |
2025-12-07T19:57:16Z |
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2025-12-07T19:57:16Z |
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