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the first method relies on comparing the measured fluxes from planetary nebulae in the sombrero galaxy to the known luminosities of planetary nebulae in the milky way.
the first method relies on comparing the measured fluxes from planetary nebulae in the sombrero galaxy to the known luminosities of planetary nebulae in the milky way.
a and b have very hot surfaces, around 32,000 and 29,600 kelvins, radiating at about 35,000 and 30,000 solar luminosities, respectively.
32.000 ve 29.600 k sıcaklıklarıyla çok sıcak yüzeylere sahiptirler ve aydınlatma güçleri (l⊙) de sırasıyla 35.000 ve 30.000'dir.
in more detail, the fri/frii division depends on host-galaxy environment in the sense that the fri/frii transition appears at higher luminosities in more massive galaxies.
daha ayrıntılı olarak, fri / frii bölünme; fri / frii geçişin daha büyük galaksilerde yüksek ışımada görünmesi bakımından, ev sahibi galaksi çevresine dayanmaktadır.