The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations
Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a sim...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Grady, C.A. [verfasserIn] |
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| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1997 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1997 |
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| Übergeordnetes Werk: |
Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 255(1997), 1-2 vom: Jan., Seite 35-41 |
|---|---|
| Übergeordnetes Werk: |
volume:255 ; year:1997 ; number:1-2 ; month:01 ; pages:35-41 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1001146314653 |
|---|
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OLC2066213624 |
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| 520 | |a Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. | ||
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| 700 | 1 | |a Pérez, M.R. |4 aut | |
| 700 | 1 | |a Bjorkman, K.S. |4 aut | |
| 700 | 1 | |a Sitko, M.L. |4 aut | |
| 700 | 1 | |a Thé, P.S. |4 aut | |
| 700 | 1 | |a De Winter, D. |4 aut | |
| 700 | 1 | |a Grinin, V.P. |4 aut | |
| 700 | 1 | |a Russell, R.W. |4 aut | |
| 700 | 1 | |a Lynch, D.K. |4 aut | |
| 700 | 1 | |a Hanner, M.S. |4 aut | |
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10.1023/A:1001146314653 doi (DE-627)OLC2066213624 (DE-He213)A:1001146314653-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Grady, C.A. verfasserin aut The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. Dust Silicate Simple Correlation Profile Shape Emission Profile Pérez, M.R. aut Bjorkman, K.S. aut Sitko, M.L. aut Thé, P.S. aut De Winter, D. aut Grinin, V.P. aut Russell, R.W. aut Lynch, D.K. aut Hanner, M.S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 255(1997), 1-2 vom: Jan., Seite 35-41 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:255 year:1997 number:1-2 month:01 pages:35-41 https://doi.org/10.1023/A:1001146314653 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 255 1997 1-2 01 35-41 |
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10.1023/A:1001146314653 doi (DE-627)OLC2066213624 (DE-He213)A:1001146314653-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Grady, C.A. verfasserin aut The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. Dust Silicate Simple Correlation Profile Shape Emission Profile Pérez, M.R. aut Bjorkman, K.S. aut Sitko, M.L. aut Thé, P.S. aut De Winter, D. aut Grinin, V.P. aut Russell, R.W. aut Lynch, D.K. aut Hanner, M.S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 255(1997), 1-2 vom: Jan., Seite 35-41 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:255 year:1997 number:1-2 month:01 pages:35-41 https://doi.org/10.1023/A:1001146314653 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 255 1997 1-2 01 35-41 |
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10.1023/A:1001146314653 doi (DE-627)OLC2066213624 (DE-He213)A:1001146314653-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Grady, C.A. verfasserin aut The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. Dust Silicate Simple Correlation Profile Shape Emission Profile Pérez, M.R. aut Bjorkman, K.S. aut Sitko, M.L. aut Thé, P.S. aut De Winter, D. aut Grinin, V.P. aut Russell, R.W. aut Lynch, D.K. aut Hanner, M.S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 255(1997), 1-2 vom: Jan., Seite 35-41 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:255 year:1997 number:1-2 month:01 pages:35-41 https://doi.org/10.1023/A:1001146314653 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 255 1997 1-2 01 35-41 |
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10.1023/A:1001146314653 doi (DE-627)OLC2066213624 (DE-He213)A:1001146314653-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Grady, C.A. verfasserin aut The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations 1997 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1997 Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. Dust Silicate Simple Correlation Profile Shape Emission Profile Pérez, M.R. aut Bjorkman, K.S. aut Sitko, M.L. aut Thé, P.S. aut De Winter, D. aut Grinin, V.P. aut Russell, R.W. aut Lynch, D.K. aut Hanner, M.S. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 255(1997), 1-2 vom: Jan., Seite 35-41 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:255 year:1997 number:1-2 month:01 pages:35-41 https://doi.org/10.1023/A:1001146314653 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2279 GBV_ILN_2286 GBV_ILN_4012 GBV_ILN_4027 GBV_ILN_4046 AR 255 1997 1-2 01 35-41 |
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The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations |
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The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations |
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Grady, C.A. |
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Astrophysics and space science |
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1997 |
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Grady, C.A. Pérez, M.R. Bjorkman, K.S. Sitko, M.L. Thé, P.S. De Winter, D. Grinin, V.P. Russell, R.W. Lynch, D.K. Hanner, M.S. |
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10.1023/A:1001146314653 |
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520 530 620 |
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the intermittently embedded herbig ae/be stars iso and ground-based ir observations |
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The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations |
| abstract |
Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. © Kluwer Academic Publishers 1997 |
| abstractGer |
Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. © Kluwer Academic Publishers 1997 |
| abstract_unstemmed |
Abstract We discuss silicate emission profiles observed with the ISO SWS and ground-based IR observations in a population of intermittently embedded Herbig Ae/Be stars which are viewed edge-on to their polarimetrically identified dust and gas disks. The ISO SWS observations confirm the lack of a simple correlation between system age and the profile shape. Comparison with laboratory silicates suggests that much of the observed variation is due to different annealing histories of the grains. © Kluwer Academic Publishers 1997 |
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The Intermittently Embedded Herbig Ae/Be Stars ISO and Ground-Based IR Observations |
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Pérez, M.R. Bjorkman, K.S. Sitko, M.L. Thé, P.S. De Winter, D. Grinin, V.P. Russell, R.W. Lynch, D.K. Hanner, M.S. |
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