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Near-IR observations of the SSV 13, SSV 9, SSV 5 sources in NGC 1333

Published online by Cambridge University Press:  04 August 2017

M. Busso ,
P. Persi ,
M. Robberto ,
F. Scaltriti  and
G. Silvestro
M. Busso
Affiliation:
(1) Osservatorio Astronomico di Pino Torinese, Torino, Italy
P. Persi
Affiliation:
(2) Istituto di Astrofisica Spaziale del C.N.R., Frascati, Italy
M. Robberto
Affiliation:
(3) Istituto di Fisica Generale dell'Università, Torino, Italy
F. Scaltriti
Affiliation:
(1) Osservatorio Astronomico di Pino Torinese, Torino, Italy
G. Silvestro
Affiliation:
(3) Istituto di Fisica Generale dell'Università, Torino, Italy

Abstract

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The sources (1) SSV 13 (identified with the IRAS (2) source 03259+3105), SSV 9 (IRAS 03256+3107), SSV 5 (IRAS 03262+3108) were observed photometrically in the JHKL bands with the In-Sb photometer at the Italian IR Telescope (TIRGO, Gornergrat, Switzerland). In addition CVF spectrophotometry between 2.0 and 2.4 μm of SSV 13 was carried out. We present a study of the energy distribution between 1 and 100 μm, including both our photometry and IRAS data.

Type
Bipolar Flows, Jets and Protostars
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 113 - 114
Copyright
Copyright © Reidel 1987 

References

Literature

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3. Cohen, M. and Schwartz, R.D. Astrophys. J., 265, 877 (1983).CrossRefGoogle Scholar