|Author||Becklin, E. E. ♦ Neugebauer, G.|
|Source||United States Department of Energy Office of Scientific and Technical Information|
|Publisher||Institute of Physics (IOP)|
|Subject Keyword||ASTRONOMY AND ASTROPHYSICS ♦ MILKY WAY- MAPS ♦ EMISSION ♦ INFRARED RADIATION ♦ LUMINOSITY ♦ PHOTOMETRY ♦ PLANETARY NEBULAE ♦ RADIOWAVE RADIATION ♦ SPATIAL RESOLUTION|
|Abstract||Photometric maps of the central 1' of the galactic center are presented at 2.2 and 10 μ with a spatial resolution of approx.2''. <sub>5</sub>. Most of the 2.2-μ radiation within the central 2 pc comes from discrete sources with absolute 2.2-μ magnitudes brighter than -8. At 10 μ, nine discrete sources plus an extended ridge of emission are seen. Five of the discrete sources are located within the extended ridge and have linear dimensions and 10-μ luminosities similar to the planetary nebula NGC 7027.|
|Learning Resource Type||Article|
|Publisher Department||Hale Observatories, California Institute of Technology, Carnegie Institution of Washington|
|Publisher Place||United States|
|Organization||Hale Observatories, California Institute of Technology, Carnegie Institution of Washington|
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