出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The Planck mission may, in principle, have a large impact on stellar studies because it will cover
a very important observational band. For various classes of stellar objects continuum observations
at millimetric and submillimetric wavelengths would be very fruitful, because they provide
essential clues to understand the physics of these stars and constitute a powerful addition to current
studies, which are carried out mostly at centimetric wavelengths. However, the high level of
galactic confusion together with the intrinsic low flux density make the detection of such kinds
of source quite challenging. In this paper we present first results of a feasibility study aimed
to investigate on the possibility to observe with Planck evolved galactic objects belonging to a
evolutionary phase that strongly influences the chemical evolution of the Galaxy
