L1014
From Wikipedia, the free encyclopedia
|
L1014 |
|
| Observation data Epoch J2000 |
|
|---|---|
| Constellation (pronunciation) |
Cygnus |
| Right ascension | 21h 24m 06s |
| Declination | +49° 59' 6"' |
| Apparent magnitude (V) | 14.2 |
| Characteristics | |
| U-B color index | ? |
| B-V color index | ? |
| Variable type | None |
| Astrometry | |
| Distance | 652.32 Ly (200 pc) |
| Details | |
| Mass | 3.6 M☉ |
| Radius | ? R☉ |
| Surface gravity (log g) | ? |
| Luminosity | 0.09 L☉ |
| Temperature | ? K |
| Metallicity | ? |
| Rotation | ? |
| Age | 10 000 - 100 000 years years |
| Other designations | |
| Database references | |
| SIMBAD | data |
L1014 is very young. "A comparison of the radial extinction profile of L1014 with other cores suggests that L1014 may be among the most centrally condensed cores known, perhaps indicative of the earliest stages of brown dwarf or star formation processes."
[edit] Reference
- http://www.journals.uchicago.edu/doi/abs/10.1086/498742
- http://jumk.de/astronomie/special-stars/l1014.shtml
- http://www.stsci.edu/observing/phase2-public/10603.pro
- http://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/full/2005/33/aa2411-04/aa2411-04.fig.html
- http://cfa-www.harvard.edu/sirtf-c2d-cfa/CORES-DB/L1014/L1014.html
- http://www.spitzer.caltech.edu/Media/releases/ssc2004-20/ssc2004-20a.shtml

