Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources (2013)
- Authors:
- Autor USP: MORENO, JORGE LUIS MELENDEZ - IAG
- Unidade: IAG
- DOI: 10.1093/mnras/stt1202
- Subjects: GALÁXIAS; ABUNDÂNCIAS (ASTRONOMIA); COSMOLOGIA; ESTRUTURA DO UNIVERSO
- Language: Inglês
- Imprenta:
- Source:
- Título: Monthly Notices of the Royal Astronomical Society
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: v. 434, p. 2572-2581, 2013
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
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ABNT
HAYWARD, Christopher C et al. Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources. Monthly Notices of the Royal Astronomical Society, v. 434, p. 2572-2581, 2013Tradução . . Disponível em: https://doi.org/10.1093/mnras/stt1202. Acesso em: 23 jan. 2026. -
APA
Hayward, C. C., Behroozi, P. S., Somerville, R. S., Primack, J. R., Moreno, J. L. M., & Wechsler, R. H. (2013). Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources. Monthly Notices of the Royal Astronomical Society, 434, 2572-2581. doi:10.1093/mnras/stt1202 -
NLM
Hayward CC, Behroozi PS, Somerville RS, Primack JR, Moreno JLM, Wechsler RH. Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 434 2572-2581.[citado 2026 jan. 23 ] Available from: https://doi.org/10.1093/mnras/stt1202 -
Vancouver
Hayward CC, Behroozi PS, Somerville RS, Primack JR, Moreno JLM, Wechsler RH. Spatially unassociated galaxies contribute significantly to the blended submillimetre galaxy population: predictions for follow-up observations of ALMA sources [Internet]. Monthly Notices of the Royal Astronomical Society. 2013 ; 434 2572-2581.[citado 2026 jan. 23 ] Available from: https://doi.org/10.1093/mnras/stt1202 - TI II λ 5380 Å as a spectroscopy indicator of stellar rotational period
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Informações sobre o DOI: 10.1093/mnras/stt1202 (Fonte: oaDOI API)
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