Source: Royal Astronomical Society. Monthly Notices. Unidades: IAG, EACH
Subjects: FORMAÇÃO DE ESTRELAS, MEIO INTERESTELAR
ABNT
AKHTER, Shaila; HARVEY-SMITH, Lisa; NAWAZ, Mohammad Ali; 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, Oxford, p. 01-29, 2020. Disponível em: < https://doi.org/10.1093/mnras/staa267 > DOI: 10.1093/mnras/staa267.APA
Akhter, S., Harvey-Smith, L., Nawaz, M. A., Jones, P. A., Walsh, A., Dal Pino, E. M. de G., 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/staa267NLM
Akhter S, Harvey-Smith L, Nawaz MA, Jones PA, Walsh A, Dal Pino EM de G, Falceta Gonçalves DA, Cunningham MR. 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.Available from: https://doi.org/10.1093/mnras/staa267Vancouver
Akhter S, Harvey-Smith L, Nawaz MA, Jones PA, Walsh A, Dal Pino EM de G, Falceta Gonçalves DA, Cunningham MR. 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.Available from: https://doi.org/10.1093/mnras/staa267