| Object | RA (J2000) | DEC (J2000) | SpTy | Category | Distance (pc) | R band (mag) | Inclination | PAdisk | Disk Diameter (") | Disk Diameter (AU) | Reference | How well Resolved | Reference Wavelength (micron) |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Haro 6-13 | 04 32 15.41 | +24 28 59.7 | M0 | YSO | 140 | 15 | 40 | 90 | 2.57 | 359.8 | Schaefer et al. 2009 | 1.8 | 1300 |
| 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 |