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Why Can We Detect Quasar BR1202-0725 in Co ?
[article]
1997
arXiv
pre-print
We present CO luminosity evolution of both elliptical and spiral galaxies based on a galactic wind model and a bulge-disk model, respectively. We have found that the CO luminosity peaks around the epoch of galactic wind caused by collective supernovae ∼ 0.85 Gyr after the birth of the elliptical with M = 2 · 10^12 M_ while ∼ 0.36 Gyr after the birth of the bulge with M = 2 · 10^11 M_. After these epochs, the CO luminosity decreases abruptly because the majority of molecular gas was expelled
arXiv:astro-ph/9710192v1
fatcat:ovvnebvypngpfos2pii33rze5q