Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS (2020)
- Authors:
- USP affiliated authors: DAL PINO, ELISABETE MARIA DE GOUVEIA - IAG ; GONÇALVES, DIEGO ANTONIO FALCETA - EACH
- Unidades: IAG; EACH
- DOI: 10.1093/mnras/staa267
- Subjects: FORMAÇÃO DE ESTRELAS; MEIO INTERESTELAR
- Language: Inglês
- Imprenta:
- Source:
- Título: Royal Astronomical Society. Monthly Notices
- ISSN: 0035-8711
- Volume/Número/Paginação/Ano: on-line, p. 01-29, 2020
- Este periódico é de assinatura
- Este artigo NÃO é de acesso aberto
- Cor do Acesso Aberto: closed
-
ABNT
AKHTER, Shaila et al. Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS. Royal Astronomical Society. Monthly Notices, p. 01-29, 2020Tradução . . Disponível em: https://doi.org/10.1093/mnras/staa267. Acesso em: 30 dez. 2025. -
APA
Akhter, S., Cunningham, M. R., Harvey-Smith, L., Nawaz, M. A., Jones, P. A., Walsh, A., et al. (2020). Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS. Royal Astronomical Society. Monthly Notices, 01-29. doi:10.1093/mnras/staa267 -
NLM
Akhter S, Cunningham MR, Harvey-Smith L, Nawaz MA, Jones PA, Walsh A, Dal Pino EM de G, Gonçalves DAF. Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS [Internet]. Royal Astronomical Society. Monthly Notices. 2020 ; 01-29.[citado 2025 dez. 30 ] Available from: https://doi.org/10.1093/mnras/staa267 -
Vancouver
Akhter S, Cunningham MR, Harvey-Smith L, Nawaz MA, Jones PA, Walsh A, Dal Pino EM de G, Gonçalves DAF. Do dense molecular cores with broad emission spectra at |l| ≈ 5.4○, |b| ≈ 0.4○ trace the Galactic bar? A multi molecular line study from HOPS [Internet]. Royal Astronomical Society. Monthly Notices. 2020 ; 01-29.[citado 2025 dez. 30 ] Available from: https://doi.org/10.1093/mnras/staa267 - Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps
- Features of collisionless turbulence in the intracluster medium from simulated Faraday rotation maps – II. The effects of instabilities feedback
- Ambient magnetic field amplification in shock fronts of relativistic jets: an application to GRB afterglows
- Relativistic MHD simulations of magnetized jets
- Turbulence and dynamo interlinks
- The ASTRI Mini-Array of cherenkov telescopes at the observatorio del teide
- Dynamo in the Intra-Cluster Medium: simulation of CGL-MHD turbulent dynamo
- MHD turbulence in the intracluster medium
- MHD turbulence-Star Formation Connection: from pc to kpc scales
- Magnetic field amplification and evolution in turbulent collisionless magnetohydrodynamics: an application to the intracluster medium
Informações sobre o DOI: 10.1093/mnras/staa267 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
