# name
Classiﬁcation of young stellar objects by CCD’s and SED’s

# metadata.dc.description[].value
Treballs Finals de Grau de Física, Facultat de Física, Universitat de Barcelona, Curs: 2021, Tutora: Maria Rosario Isabel López Hermoso

# metadata.dc.description.abstract[].value
The purpose of this study was to classify 19 Infrared Astronomical Satellite (IRAS) sources located in Cepheus molecular cloud. We have taken these sources because all have an CO outﬂow emission, which is an important tracer of star-formation process. We have obtained the ﬂux of these protostars from the IRAS, Spitzer, WISE and 2MASS catalogs at far, medium and near infrared wavelenghts (FIR, MIR, NIR) to compute: color-color diagrams (CCD’s) according to determine the evolutionary Class at which the IRAS sources belong to, and the spectral distribution of energy (SED) with the aim of check and complete the previous classiﬁcation. We found 13 sources belonging to Class 0, 3 to Class I, 3 to Class 0/I and none of Class II and III

# metadata.dc.title[].value
Classiﬁcation of young stellar objects by CCD’s and SED’s