About: Delayed recombination as a major source of the soft X-ray background

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scientific article published in Nature

Attributes	Values
rdf:type	Item
description	artículu científicu (ast) wetenschappelijk artikel (nl) bài báo khoa học (vi) article publié dans la revue scientifique Nature (fr) im Oktober 1994 veröffentlichter wissenschaftlicher Artikel (de) scientific article published in Nature (en) наукова стаття, опублікована в Nature в жовтні 1994 (uk)
publication date	wds:Q60071420-900F4D41-9186-4985-B2BF-96663D2C7768
publication date	1994-10-01 00:00:00Z (xsd:dateTime)
language of work or name	wds:Q60071420-A1DB478B-5C2E-4D29-8801-EFC2E1FDECB7
language of work or name	English
exact match	wds:Q60071420-893DA3D2-E869-49F6-97E4-4B72EE577D22
exact match	https://scigraph.springernature.com/pub.10.1038/371774a0
cites work	wds:Q60071420-02436951-B07F-4CFC-B33F-CC92E050358D wds:Q60071420-44BAF6BF-5B54-4074-A698-3518EAB5134A wds:Q60071420-4730EA44-0317-4D77-9D40-D942468492FC wds:Q60071420-547DC240-2279-4164-BAC1-1EE07CAE4944 wds:Q60071420-55E45DC0-A9CD-48BB-9DE3-9658AEB9D931 wds:Q60071420-75E11130-E050-402C-B175-7D04CAADA4BE wds:Q60071420-8C3E311A-6030-45A8-A41E-D45430C09E4D wds:Q60071420-90E926EE-C274-4916-B0C4-EF230F9192B0 wds:Q60071420-9A8DBFDD-80FA-4918-9EB9-10B0D60C0D05 wds:Q60071420-A28E9935-D2ED-49E6-9B97-E51CB7AE6EC6 wds:Q60071420-C4519EB7-5C00-4DF1-8E9D-92D7B8FB8EEE wds:Q60071420-D1F17E04-DA5F-41F8-913C-2B112C0A250F wds:Q60071420-D7C61E5D-63FF-46A3-B510-C44B7BF23AF5 wds:Q60071420-DAD90CFF-71D9-4D94-B97C-4EE930EA722C wds:Q60071420-F104FD81-3C65-422B-88CB-94E543D30536
cites work	On the origin of the soft X-ray background Detection of an Anisotropic Soft X-ray Background Flux The O Associations in the Solar Neighborhood On the distribution of interstellar matter around the sun What ionizes the interstellar hydrogen toward PSR 0950+08 and PSR 0823+26 ? A model for the distribution of material generating the soft X-ray background The exceptionally vacant line of sight to beta Canis Majoris Supershells and propagating star formation Discovery of a very bright, nearby binary millisecond pulsar The HI halo in the inner galaxy The soft X-ray diffuse background Clustered supernovae versus the gaseous disk and halo Star formation rates and abundance gradients in disk galaxies The X-ray shadow of the high-latitude molecular cloud MBM 12 Stellar winds in HII regions - II. Turbulent mixing between an HII layer and a stellar wind bubble in the presence of a magnetic field
author name string	wds:Q60071420-761AA2EC-8659-4C64-AAFB-03A3B1CA4CE7 wds:Q60071420-E4623120-72D9-4208-9EFD-CA29C5151DB7
author name string	D. Breitschwerdt T. Schmutzler
rdfs:label	Delayed recombination as a major source of the soft X-ray background (en) Delayed recombination as a major source of the soft X-ray background (nl)
skos:prefLabel	Delayed recombination as a major source of the soft X-ray background (en) Delayed recombination as a major source of the soft X-ray background (nl)
name	Delayed recombination as a major source of the soft X-ray background (en) Delayed recombination as a major source of the soft X-ray background (nl)
title	wds:Q60071420-453B741E-4EC3-4933-8B1A-25E9D91F05A0
title	Delayed recombination as a major source of the soft X-ray background (en)
page(s)	wds:Q60071420-2A6C5C68-4B2D-4C20-8EBE-0F273988D848
page(s)	774-777
instance of	wds:Q60071420-6FF1CDB3-0AB9-4A18-BBD7-97D26FA30D95
instance of	scholarly article
published in	wds:Q60071420-33189FD7-EB8D-488A-9FE7-A08E3BA9EFF1
published in	Nature
issue	wds:Q60071420-E0CBF03B-CE3F-4134-8714-BD3B8B07BD7D
volume	wds:Q60071420-0D021592-3EF9-4CEA-A380-920CF6F7E736
issue	6500
volume	371
DOI	wds:Q60071420-197A374C-53B5-4AB7-9639-68C94B56488D
DOI	http://dx.doi.org/10.1038/371774A0
DOI	10.1038/371774A0
Dimensions Publication ID	wds:Q60071420-06BB78C6-1778-475A-AE40-862C2670DE58
Dimensions Publication ID	1039300819
is about of	https://www.wikidata.org/wiki/Special:EntityData/Q60071420
is cites work of	The gradient of diffuse {gamma}-ray emission in the Galaxy Far Ultraviolet Spectroscopic Explorer (FUSE) observations of emitting and absorbing gas in the Local Interstellar Chimney
is cites work of	wds:Q68512340-B7E59F69-B6B8-4F4A-99A7-2F380F1B2A8C wds:Q68510871-9E1B1643-6DD2-4611-9C7E-4FADE7F1F7ED

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