Wisconsin Astrophysics, Issues 91-105Washburn Observatory, University of Wisconsin., 1979 - Astronomy |
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... temperature had dropped to 1500 K. -1 ( An adiabatic shock moving at 15 km s produces temperatures around 6000 K. ) Thereafter the temperature dropped more slowly , not reaching 200 K for another 1.43 time units . Figure 2 shows a ...
... temperature had dropped to 1500 K. -1 ( An adiabatic shock moving at 15 km s produces temperatures around 6000 K. ) Thereafter the temperature dropped more slowly , not reaching 200 K for another 1.43 time units . Figure 2 shows a ...
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... temperature and thickness to that seen along ~ 30 ° , a factor of 2 less in the pressure ( electron density ) would explain why a ridge along 270 ° was not detected in past experiments . If the spectral hardening seen at the outer ...
... temperature and thickness to that seen along ~ 30 ° , a factor of 2 less in the pressure ( electron density ) would explain why a ridge along 270 ° was not detected in past experiments . If the spectral hardening seen at the outer ...
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... temperature of ex the main hf component ( assumed to be the same for all hf components of N = 10 ) , TCB is the cosmic background brightness temperature ( 2.7K ) , Tc is the background brightness temperature of any discrete source which ...
... temperature of ex the main hf component ( assumed to be the same for all hf components of N = 10 ) , TCB is the cosmic background brightness temperature ( 2.7K ) , Tc is the background brightness temperature of any discrete source which ...
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30 Doradus 5000 WAVELENGTH HD 5000 WAVELENGTH WAVELENGTH absorption albedo Ap.J array Astr B2 IV-V background calculations carbon band channel color excess column densities components cooling count rates curve derived detected disk DISK2 emission lines equation estimate extinction feature Figure flux galactic H II region H₂ header hydrogen indicated infrared intensity interstellar interstellar extinction ionization front km s¹ Koornneef line profiles log F(X luminosity Magellanic Cloud maps mass loss measurements molecular clouds nebula observed optical photons pixel plotted radial velocity radio continuum rate of mass resolution Reticon ridge Savage scans shocked layer spectra spectral type spectrum stellar stellar wind Table tape temperature ultraviolet University of Wisconsin-Madison Uranus VLSR Washburn Observatory WAVELENGTH 2.5 log WAVELENGTH 5000 X-ray ΙΑ