Portal de Periódicos da CAPES

On the interpretation of the broad-band millimeter-wave flux from Orion

1984; IOP Publishing; Volume: 283; Linguagem: Inglês

10.1086/184329

1538-4357

E. C. Sutton, Geoffrey A. Blake, C. R. Masson, T. G. Phillips,

Molecular Spectroscopy and Structure

view Abstract Citations (60) References (8) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS On the interpretation of the broad-band millimeter-wave flux from Orion. Sutton, E. C. ; Blake, G. A. ; Masson, C. R. ; Phillips, T. G. Abstract Spectral observations of the core of Orion A at wavelengths around 1.3 mm show a high density of strong, broad emission lines. The combined flux in lines with peak antenna temperatures stronger than 0.2 K accounts for approximately 40 percent of the broad-band millimeter-wave flux from the region. Thus the broad-band flux from Orion A is in large part due to sources other than dust emission. Publication: The Astrophysical Journal Pub Date: August 1984 DOI: 10.1086/184329 Bibcode: 1984ApJ...283L..41S Keywords: Millimeter Waves; Molecular Clouds; Orion Nebula; Radio Astronomy; Broadband; Emission Spectra; Flux Density; Astrophysics full text sources ADS | data products SIMBAD (2)