Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities (1994)
Fonte: Astrophysics and Space Science. Unidade: IAG
Assuntos: ASTRONOMIA, ESTRELAS (CLASSIFICAÇÃO)
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
ABNT
ROSSI, Silvia Cristina Fernandes et al. Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities. Astrophysics and Space Science, v. 213, n. 1, p. 113-119, 1994Tradução . . Disponível em: https://doi.org/10.1007/bf00627781. Acesso em: 03 maio 2024.APA
Rossi, S. C. F., Barbuy, B. L. S., Pineau des Forets, G., & Benevides-Soares, P. (1994). Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities. Astrophysics and Space Science, 213( 1), 113-119. doi:10.1007/bf00627781NLM
Rossi SCF, Barbuy BLS, Pineau des Forets G, Benevides-Soares P. Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities [Internet]. Astrophysics and Space Science. 1994 ; 213( 1): 113-119.[citado 2024 maio 03 ] Available from: https://doi.org/10.1007/bf00627781Vancouver
Rossi SCF, Barbuy BLS, Pineau des Forets G, Benevides-Soares P. Cooling by grains and 'H IND.2' in collapsing clouds of different metallicities [Internet]. Astrophysics and Space Science. 1994 ; 213( 1): 113-119.[citado 2024 maio 03 ] Available from: https://doi.org/10.1007/bf00627781
