Výsledky vyhledávání - "ISM: individual objects: W44"
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Zdroj: Onsala rymdobservatorium infrastruktur Chockkompressioner i det interstellära mediet som triggers av Star Formation Astronomy and Astrophysics. 693
Témata: ISM: supernova remnants, ISM: individual objects: W44, ISM: molecules, ISM: bubbles, ISM: individual objects: G034.77-00.55, ISM: clouds
Popis souboru: electronic
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Zdroj: Chockkompressioner i det interstellära mediet som triggers av Star Formation Star formation history of MAssive pRoTostars (SMART) Astronomy and Astrophysics. 675
Témata: ISM: individual objects: G34.77-00.55, ISM: individual objects: W44, Stars: formation, ISM: clouds, ISM: supernova remnants, Astrochemistry
Popis souboru: electronic
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Zdroj: Astronomy & Astrophysics , 675 , Article A190. (2023)
Témata: astrochemistry, ISM: clouds, ISM: supernova remnants, ISM: individual objects: G34.77-00.55, ISM: individual objects: W44, stars: formation
Popis souboru: text
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Témata: Ism: Individual Objects: Ic 443, Ism: Individual Objects: W44, Ism: Supernova Remnants, 天文学, 天文学::恒星与银河系, Astronomy & Astrophysics, DIFFUSIVE SHOCK ACCELERATION, EMISSION, IC-443, TELESCOPE, PARTICLES, PROTONS, WAVES, DENSE, GAS, W28, Science & Technology, Physical Sciences, 理学, 理学::天文学
Relation: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY; http://ir.ynao.ac.cn/handle/114a53/9424; http://mnras.oxfordjournals.org/content/435/1/570
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Témata: ISM: individual objects: W44, ISM: supernova remnants, Radio continuum: ISM, Data reduction, Mathematical models, Natural frequencies, Optical resolving power, Sensitivity analysis, Spectrum analysis, Individual objects, ISM, Radio continuum, Supernova remnants, Signal to noise ratio
Relation: https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_00046361_v471_n2_p537_Castelletti; https://hdl.handle.net/20.500.12110/paper_00046361_v471_n2_p537_Castelletti
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Témata: Astrochemistry, ISM: clouds, ISM: individual objects: G34.77-00.55, ISM: individual objects: W44, ISM: supernova remnants, Stars: formation, artículo
URL:
http://hdl.handle.net/10261/357594
Publisher's versionhttp://dx.doi.org/10.1051/0004-6361/202346676
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info:eu-repo/grantAgreement/EC/H2020/788829
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2019-105552RB-C41/ES/CONTRIBUCION DEL CAB A SPICA, DESARROLLO DE INSTRUMENTACION CRIOGENICA Y EXPLOTACION CIENTIFICA MULTILONGITUD DE ONDA
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-114461GB-I00/ES/SISTEMAS PLANETARIOS A LO LARGO DE LA EVOLUCION ESTELAR
info:eu-repo/grantAgreement/AEI/Programa Estatal para Impulsar la Investigación Científico-Técnica y su Transferencia 2021-2023/CEX2021-001131-S
info:eu-repo/grantAgreement/EC/H2020/833460 -
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ANALYTIC SOLUTION FOR SELF-REGULATED COLLECTIVE ESCAPE OF COSMIC RAYS FROM THEIR ACCELERATION SITES.
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Zdroj: The Astrophysical journal [Astrophys J] 2013 May 01; Vol. 768 (1). Date of Electronic Publication: 2013 Apr 16.
Způsob vydávání: Journal Article
Informace o časopise: Publisher: Published by the University of Chicago Press for the American Astronomical Society Country of Publication: United States NLM ID: 9890633 Publication Model: Print-Electronic Cited Medium: Print ISSN: 0004-637X (Print) Linking ISSN: 0004637X NLM ISO Abbreviation: Astrophys J Subsets: PubMed not MEDLINE
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