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Near-infrared and optical observations of IRAS sources in and near dense cores

Myers, P. C., Fuller, Gary A., Mathieu, R. D., Beichman, C. A., Benson, P. J., Schild, R. E., Emerson, J. P.·1987·The Astrophysical Journal

Abstract

The authors report photometry from 0.4 to 20 μm of 34 IRAS point sources associated with dense cores in dark clouds. The main results of this study are: (1) Stars near cores tend to be visible T Tauri stars, while stars in cores tend to have circumstellar extinction AV ≡ 30 - 90 mag and luminosity ≡1 L_sun;, similar to that of T Tauri stars. (2) The typical highly obscured star is probably accompanied by a luminous structure of substellar temperature, such as a circumstellar disk. (3) In Taurus-Aurigae, stars in cores probably become visible T Tauri stars less than 1×105yr after they attain luminosity greater than ≡0.1 L_sun;. This implies that they are extremely young and may still be accreting.

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Metadata

Authors
Myers, P. C., Fuller, G. A., Mathieu, R. D., Beichman, C. A., Benson, P. J., Schild, R. E., & Emerson, J. P.
Venue
The Astrophysical Journal
Published
1987-08
Volume
319
Pages
340
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1999263013
Cited by
265
References
0
FWCI
11.31
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Near-infrared and optical observations of IRAS sources in and near dense cores. https://app.cochat.ai/papers/10.1086/165458
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Myers, P. C., Fuller, G. A., Mathieu, R. D., Beichman, C. A., Benson, P. J., Schild, R. E., & Emerson, J. P. (1987). Near-infrared and optical observations of IRAS sources in and near dense cores. The Astrophysical Journal. https://doi.org/10.1086/165458

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