Epoch J2000 Equinox J2000
|Right ascension||07h 13m 22.55s|
|Declination||−29° 17′ 51.9″|
|Apparent magnitude (J (MKO-NIR filter system))||19.64 ± 0.15|
|Apparent magnitude (J (SOAR/OSIRIS))||20.06 ± 0.21|
|Apparent magnitude (H (MKO-NIR filter system))||>19.3|
|Apparent magnitude (H (SOAR/OSIRIS))||21.16 ± 0.66|
|Distance||~ 23.2 ly
(~ 7.1 pc)
WISE 0713−2917 was discovered in 2012 by J. Davy Kirkpatrick and colleagues from data collected by the Wide-field Infrared Survey Explorer (WISE) in the infrared at a wavelength of 40 cm (16 in), whose mission lasted from December 2009 to February 2011. In 2012 Kirkpatrick et al. published a paper in The Astrophysical Journal, where they presented discovery of seven new found by WISE brown dwarfs of spectral type Y, among which also was WISE 0713−2917.
Trigonometric parallax of WISE 0713−2917 is not yet measured. Therefore, there are only distance estimates of this object, obtained by indirect—spectrophotometric—means (see table).
WISE 0713−2917 distance estimates
|Source||Parallax, mas||Distance, pc||Distance, ly||Ref.|
|Kirkpatrick et al. (2012), Tables 4 & 8||7.1||23.2|||
Non-trigonometric distance estimates are marked in italic.
The other six discoveries of brown dwarfs, published in Kirkpatrick et al. (2012):
- WISE 0146+4234 (Y0)
- WISE 0350−5658 (Y1)
- WISE 0359−5401 (Y0)
- WISE 0535−7500 (≥Y1)
- WISE 0734−7157 (Y0)
- WISE 2220−3628 (Y0)
- Kirkpatrick, J. D.; Gelino, C. R.; Cushing, M. C.; Mace, G. N.; Griffith, R. L.; Skrutskie, M. F.; Marsh, K. A.; Wright, E. L.; Eisenhardt, P. R.; McLean, I. S.; Mainzer, A. K.; Burgasser, A. J.; Tinney, C. G.; Parker, S.; Salter, G. (2012). "Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function". The Astrophysical Journal. 753 (2): 156. Bibcode:2012ApJ...753..156K. arXiv: . doi:10.1088/0004-637X/753/2/156.
|This brown dwarf-related article is a stub. You can help Wikipedia by expanding it.|