BN objects — A class of very young and massive stars
Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1986 |
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| Umfang: |
18 |
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| Reproduktion: |
Springer Online Journal Archives 1860-2002 |
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| Übergeordnetes Werk: |
in: Astrophysics and space science - 1968, 128(1986) vom: Jan., Seite 199-216 |
| Übergeordnetes Werk: |
volume:128 ; year:1986 ; month:01 ; pages:199-216 ; extent:18 |
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| 520 | |a Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. | ||
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(DE-627)NLEJ193016141 DE-627 ger DE-627 rakwb eng BN objects — A class of very young and massive stars 1986 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. Springer Online Journal Archives 1860-2002 Henning, Th. oth Gürtler, J. oth in Astrophysics and space science 1968 128(1986) vom: Jan., Seite 199-216 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:128 year:1986 month:01 pages:199-216 extent:18 http://dx.doi.org/10.1007/BF00656030 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 128 1986 1 199-216 18 |
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(DE-627)NLEJ193016141 DE-627 ger DE-627 rakwb eng BN objects — A class of very young and massive stars 1986 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. Springer Online Journal Archives 1860-2002 Henning, Th. oth Gürtler, J. oth in Astrophysics and space science 1968 128(1986) vom: Jan., Seite 199-216 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:128 year:1986 month:01 pages:199-216 extent:18 http://dx.doi.org/10.1007/BF00656030 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 128 1986 1 199-216 18 |
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(DE-627)NLEJ193016141 DE-627 ger DE-627 rakwb eng BN objects — A class of very young and massive stars 1986 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. Springer Online Journal Archives 1860-2002 Henning, Th. oth Gürtler, J. oth in Astrophysics and space science 1968 128(1986) vom: Jan., Seite 199-216 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:128 year:1986 month:01 pages:199-216 extent:18 http://dx.doi.org/10.1007/BF00656030 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 128 1986 1 199-216 18 |
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(DE-627)NLEJ193016141 DE-627 ger DE-627 rakwb eng BN objects — A class of very young and massive stars 1986 18 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. Springer Online Journal Archives 1860-2002 Henning, Th. oth Gürtler, J. oth in Astrophysics and space science 1968 128(1986) vom: Jan., Seite 199-216 (DE-627)NLEJ188985301 (DE-600)1472548-4 1572-946X nnns volume:128 year:1986 month:01 pages:199-216 extent:18 http://dx.doi.org/10.1007/BF00656030 GBV_USEFLAG_U ZDB-1-SOJ GBV_NL_ARTICLE AR 128 1986 1 199-216 18 |
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in Astrophysics and space science 128(1986) vom: Jan., Seite 199-216 volume:128 year:1986 month:01 pages:199-216 extent:18 |
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BN objects — A class of very young and massive stars |
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Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. |
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Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. |
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Abstract The Becklin-Neugebauer objects are identified by means of a wide range of observable features as a separate class of very young and massive stars surrounded by optically thick dust shells. We show that they evolutionarily connect real protostars to compactHii regions. We give criteria which should be appropriate to segregate the BN objects from compactHii regions. Finally, we describe the structure of a typical BN object. |
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