Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF
Research output: Other contribution › Research
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Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF. / Davidzon, Iary.
2017, Datasets.Research output: Other contribution › Research
Harvard
Davidzon, I 2017, Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF.. <https://www.nbi.dk/~mns551/mydata/Davidzon+17_SMD.txt>
APA
Davidzon, I. (2017). Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF. https://www.nbi.dk/~mns551/mydata/Davidzon+17_SMD.txt
Vancouver
Davidzon I. Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF. 2017.
Author
Bibtex
@misc{cf8e0ff6fa0941b4a0d33f28883b69a0,
title = "Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF",
author = "Iary Davidzon",
note = "Datasets",
year = "2017",
language = "English",
type = "Other",
}
RIS
TY - GEN
T1 - Stellar mass density from the integrated stellar mass function down to 10^9 Msol. Assuming Omega_m,Omega_L,h = 0.3,0.7,0.70 and Chabrier (2003) IMF
AU - Davidzon, Iary
N1 - Datasets
PY - 2017
Y1 - 2017
M3 - Other contribution
ER -
ID: 243194808