discov_num | notes | refcode |
RED 13 | Primary is NLTT 22741 = LP 261-75, secondary 2MASS J09510549+3558021. | |
Distance to system 28.0 +/- 5pc, upper age limit about 2.2 Gyr. It is | ||
uncertain whether the pair is physically bound. | Sef2005b | |
Reid et al. (2006) combine near-IR imaging with 2MASS data and optical | Red2006c | |
spectroscopy; conclude the stars form a CPM pair, with separation 450 | ||
+/- 120au and a distance of 38 +/- 10pc. The primary (LP 261-75) is an | ||
M4.5 dwarf; spectral type of the secondary is L6, with mass perhaps | ||
~0.02 Msun. |
refcode | metd | author | reference |
Red2006c | Ci w | Reid, I.N. & Walkowicz, L.M. | 2006PASP..118..671R |
Red2006c | +E2 | PASP 118, 671, 2006 | |
Sef2005b | Ci - | Seifahrt, A., Mugrauer, M., Wiese, M., Neuhauser, R., & Guenther, E.W. | 2005AN....326..974S |
Sef2005b | +Pa | AN 326, 974, 2005 (all measures extracted from 2MASS PSC by cataloger) |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
09511+3558 | RED 13 | 2006 | 3 | 128 | 13.4 | 10.57 | 17.22 | M4.5+L6 | N DK | 095104.57+355809.4 |