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- W3105364470 abstract "Flux calibrated images of the known supernova remnant G 34.7-0.4 in basic optical emission lines are presented. The low ionization images show a relatively flat flux distribution. The diffuse and patchy morphology of the detected optical emission may indicate the presence of turbulent magnetic fields. Typical observed H] fluxes are ~8 10-17 erg s-1 cm-2 arcsec-2, while the [] fluxes are lower around 4 10-17 erg s-1 cm-2 arcsec-2. Emission in the medium ionization line of [] 5007 Å is not detected within our sensitivity limits, probably due to the heavy extinction towards the remnant. The long-slit spectra reveal strong [] and [] emission relative to Hα and moderate [] 6300 Å emission. Shock velocities in the range of 110–150 km s-1 and low electron densities are estimated. Archival MSX infrared data show emission in the south and west areas of the remnant matching rather well the optical and radio emission." @default.
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- W3105364470 date "2003-06-19" @default.
- W3105364470 modified "2023-09-26" @default.
- W3105364470 title "The faint supernova remnant G 34.7-0.4 (W44)" @default.
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- W3105364470 doi "https://doi.org/10.1051/0004-6361:20030603" @default.
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