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Haro 6-13

RA (J2000)
DEC (J2000)
R band (mag)
Distance (pc)
Disk Diameter (")
Disk Diameter (AU)
How Well Resolved
At ref. wavelength (micron)
# References
04 32 15.41+24 28 59.7YSOM0151402.57359.84090Schaefer et al. 20091.813006



A dual-frequency sub-arcsecond study of proto-planetary disks at mm wavelengths: first evidence for radial variations of the dust properties
Guilloteau, S., Dutrey, A., Pietu, V., and Boehler, Y. 2011 A.&A. 529 A105
The Taurus Spitzer Survey: New Candidate Taurus Members Selected Using Sensitive Mid-Infrared Photometry
Rebull, L.M. et al. 2010 Ap.J.S. 186 259
A Millimeter-wave Interferometric Study of Dust and CO Disks Around Late Spectral Type Stars in Taurus-Auriga
*Schaefer, G.H. et al. 2009 Ap.J. 701 698
Circumstellar dust disks in Taurus-Auriga: The submillimeter perspective
Andrews, S.M. & Williams, J.P., 2005, ApJ, 631, 1134
On the evolutionary status of class I stars and Herbig-haro energy sources in Taurus-Auriga
White, R.J., & Hillenbrand, L.A., 2004, ApJ, 616, 998
The embedded young stars in the Taurus-Auriga molecular cloud. I - Models for spectral energy distributions
Kenyon, S.J., Calvet, N., and Hartmann, L. 1993 Ap.J. 414 676