About: HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec

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About: HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec Goto Sponge NotDistinct Permalink

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scientific article published in Astronomical Journal

Attributes	Values
rdf:type	Item
description	wetenschappelijk artikel (nl) наукова стаття, опублікована у квітні 1995 (uk) im April 1995 veröffentlichter wissenschaftlicher Artikel (de) article publié dans la revue scientifique Astronomical Journal (fr) scientific article published in Astronomical Journal (en) artículu científicu espublizáu en The Astronomical Journal (ast)
publication date	wds:Q56114555-5BA1ACF7-B871-49A2-BFC7-BAC802F21968
publication date	1995-04-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q56114555-6C5AB3AC-36B0-4DC7-BD92-5CCFCD2EDE5D
language of work or name	English
author name string	wds:Q56114555-234CC44E-01EA-41AC-892E-ED6E6674497B wds:Q56114555-2D4EE9DB-1590-4C17-9239-80428231BA37 wds:Q56114555-4EF8B600-EF4B-47A2-97CF-A9B816C661ED wds:Q56114555-74D187EC-46EE-46C5-9B22-6FB221FED624 wds:Q56114555-7BA56AF0-D8EE-48E9-BC6B-B52ADE5759A0 wds:Q56114555-A22803E5-6B51-42BD-ABA8-D86DEF99EFAB
author name string	Arsen R. Hajian Roberta M. Humphreys Kris Davidson Nolan R. Walborn Michael Rosa Dennis Ebbets
rdfs:label	HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (en) HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (nl)
skos:prefLabel	HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (en) HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (nl)
name	HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (en) HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (nl)
author	wds:Q56114555-AA36AD80-1279-4E1E-9CC7-BFC82D9B94BE
author	Gerd Weigelt
title	wds:Q56114555-B6D926FA-E40F-433E-8F31-8791A1293F08
title	HST/FOS spectroscopy of ETA Carinae: the star itself, and ejecta within 0.3 arcsec (en)
page(s)	wds:Q56114555-055288C8-2137-42A8-A8FC-10770358648A
page(s)	1784–1796
instance of	wds:Q56114555-92AC62CA-89E2-40F0-B8BC-33F1E3C6887D
instance of	scholarly article
published in	wds:Q56114555-3D07066C-3783-4DF4-B496-38332F232706
published in	The Astronomical Journal
volume	wds:Q56114555-E99ED158-AD62-4EAF-96A9-0D84C755787D
volume	109
DOI	wds:Q56114555-751D8E55-E8DC-4200-8B1A-A9F6BD310BCB
DOI	http://dx.doi.org/10.1086/117408
DOI	10.1086/117408
ResearchGate publication ID	wds:Q56114555-B8BE562E-0A90-46C2-B32A-4DFCCE8BC5DD
ResearchGate publication ID	234209936
ADS bibcode	wds:Q56114555-3508A0F3-1EE9-41A2-8FAE-7605DF2B0BFB
ADS bibcode	1995AJ....109.1784D
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q56114555
is cites work of	The periodicity of the η Carinae events Constraining the absolute orientation of η Carinae’s binary orbit: a 3D dynamical model for the broad [Fe iii] emission★ Near-infrared evidence for a sudden temperature increase in Eta Carinae Eta Carinae’s 2014.6 spectroscopic event: Clues to the long-term recovery from its Great Eruption Constraints on decreases in η Carinae's mass-loss from 3D hydrodynamic simulations of its binary colliding winds Metastable hydrogen absorption in ejecta close to $\mathsf{\eta}$ Carinae {eta} Carinae: The optical flare-like events during low-excitation passages Is eta Carinae a long-period binary? The FERRUM Project: Experimental transition probabilities of [Fe II] and astrophysical applications A model for the origin of the anomalous and very bright UV lines of Fe II in gaseous condensations of the star {eta} Carinae Time variations of the narrow Fe II and H I spectral emission lines from the close vicinity of η Carinae during the spectral event of 2003 Anomalously bright UV lines of Fe II as a probe of gas condensations in the vicinity of hot stars Radiative cycle with stimulated emission from atoms and ions in an astrophysical plasma ηCarinae: linelist for the emission spectrum of the Weigelt blobs in the 1700 to 10 400 Å wavelength region
is cites work of	wds:Q56114584-0EAC9078-137E-4D87-93AC-C9CDC774014B wds:Q56114589-6EEA711A-3C85-4261-AA18-F4146389F31A wds:Q68846044-E9C27069-5283-4C35-96B5-0D192C5C9D18 wds:Q59013830-C5BEFA2E-9E0E-46E9-8D89-7C85A1A9399E wds:Q56114558-DBAA4BE5-3735-4C9D-BEB3-5ED1CE63F798 wds:Q54255433-59F9F21F-1BDB-46B5-8DE8-377E1573430D wds:Q68842596-0C2F60FE-4886-45BB-817C-CE7E38241C81 wds:Q59013863-457ACF08-81F1-4B72-B1B2-5CD2F359B64D wds:Q68846861-B89A9941-3814-4864-B608-DE9BB860DFB9 wds:Q54255414-0FAA1BD1-A38C-4F4B-ACF0-C21FA6DFCB7E wds:Q68192896-7BD52E33-E49F-4783-A8FE-6702B545F3C3 wds:Q59013492-9A9C977B-F996-47D4-AC0D-D3E07491A123 wds:Q78897725-20C70FA9-5D47-4069-8341-7C7281A6ABC8 wds:Q59013916-B717CB3C-546A-4C9B-AAE4-775DE70E34B5

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