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scientific article published in the Astrophysical Journal

AttributesValues
rdf:type
description
  • artículu científicu (ast)
  • wetenschappelijk artikel (nl)
  • bài báo khoa học (vi)
  • article publié dans la revue scientifique Astrophysical Journal (fr)
  • наукова стаття, опублікована в лютому 2018 (uk)
  • scientific article published in the Astrophysical Journal (en)
  • im Februar 2018 veröffentlichter wissenschaftlicher Artikel (de)
publication date
publication date
language of work or name
language of work or name
author name string
author name string
  • David L. Clements
  • Douglas Scott
  • Yiping Shu
  • Hooshang Nayyeri
  • Paloma I. Martínez-Navajas
  • Camilo E. Jiménez-Ángel
rdfs:label
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (en)
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (nl)
skos:prefLabel
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (en)
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (nl)
name
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (en)
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (nl)
author
author
title
title
  • The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas (en)
page(s)
page(s)
  • 151
instance of
instance of
published in
published in
issue
volume
issue
  • 2
volume
  • 854
DOI
DOI
DOI
  • 10.3847/1538-4357/AAABB7
arXiv ID
arXiv ID
  • 1802.00242
ADS bibcode
ADS bibcode
  • 2018ApJ...854..151M
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is about of
is pr:P248 of
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