Bibcode
Mampaso, A.; Sanchez-Magro, C.; Selby, M. J.; MacGregor, A. D.
Referencia bibliográfica
Revista Mexicana de Astronomia y Astrofisica, Vol. 8, Issue 1, p. 3, 1983
Fecha de publicación:
6
1983
Número de citas
8
Número de citas referidas
7
Descripción
During the summer of 1978 the F Corona was
observed from the ground in the near infrared at 2. and 3. in an attempt
to measure the localized thermal emission from dust predicted by
Peterson (1963) and several other workers. We failed to detect this
emission even though our experimental errors were well below previously
quoted emission values. If thermal emission peaks around the sun exist,
we believe they are either much weaker or have different shapes compared
to previous ones found. This result, if confirmed, will require a
revision of the dynamics and physics of circumsolar dust.