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The nature of the embedded population in the Rho Ophiuchi dark cloud - Mid-infrared observations

Lada, C. J., Wilking, B. A.·1984·The Astrophysical Journal

Abstract

The authors present results of mid-infrared (primarily 10 and 20 μm wavelength) observations of previously identified members of the embedded populatin of the ρ Ophiuchi dark cloud. These observations enable determination of broad-band energy distributions for 32 of the 44 sources known to be embedded in the cloud. The majority of the sources emit the bulk of their luminosity between 1 μm and 20 μm. These sources apparently are surrounded by dust shells and are probably pre-main-sequence in nature. It is found that the embedded cluster is predominantly composed of low-luminosity objects with luminosities in the range 0.1 ≤ L/L_sun; ≤ 25. When corrected for observational selection effects, the resulting luminosity function appears to be deficient in intermediate-luminosity stars compared with the luminosity function for field stars.

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Metadata

Authors
Lada, C. J., & Wilking, B. A.
Venue
The Astrophysical Journal
Published
1984-12
Volume
287
Pages
610
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W2074299830
Cited by
492
References
0
FWCI
9.12
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: The nature of the embedded population in the Rho Ophiuchi dark cloud - Mid-infrared observations. https://app.cochat.ai/papers/10.1086/162719
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Lada, C. J., & Wilking, B. A. (1984). The nature of the embedded population in the Rho Ophiuchi dark cloud - Mid-infrared observations. The Astrophysical Journal. https://doi.org/10.1086/162719

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