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:	Henning, Th. [verfasserIn] Gürtler, J.

Format:	Artikel
Sprache:	Englisch

Erschienen:	1986

Schlagwörter:	Dust Massive Star Observable Feature Separate Class Dust Shell

Anmerkung:	© D. Reidel Publishing Company 1986

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 128(1986), 1 vom: Dez., Seite 199-216
Übergeordnetes Werk:	volume:128 ; year:1986 ; number:1 ; month:12 ; pages:199-216

Links:	Volltext

DOI / URN:	10.1007/BF00656030

Katalog-ID:	OLC2066163570

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spelling	10.1007/BF00656030 doi (DE-627)OLC2066163570 (DE-He213)BF00656030-p DE-627 ger DE-627 rakwb eng 520 530 620 VZ 16,12 ssgn Henning, Th. verfasserin aut BN objects — A class of very young and massive stars 1986 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © D. Reidel Publishing Company 1986 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. Dust Massive Star Observable Feature Separate Class Dust Shell Gürtler, J. aut Enthalten in Astrophysics and space science Kluwer Academic Publishers, 1968 128(1986), 1 vom: Dez., Seite 199-216 (DE-627)129062723 (DE-600)629-4 (DE-576)014393522 0004-640X nnns volume:128 year:1986 number:1 month:12 pages:199-216 https://doi.org/10.1007/BF00656030 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_24 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_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 AR 128 1986 1 12 199-216
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title_auth	BN objects — A class of very young and massive stars
abstract	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. © D. Reidel Publishing Company 1986
abstractGer	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. © D. Reidel Publishing Company 1986
abstract_unstemmed	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. © D. Reidel Publishing Company 1986
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BN objects — A class of very young and massive stars

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