I recently read about a pair of brown dwarfs found in space.com.(http://www.space.com/astronotes/astronotes.html).
One which has 25 Jupiter masses and the other with 50 Jupiter masses.Is it a possible addition to extrasolar.ssc or not?Since they are not orbiting a normal star,it?s difficult to say if it go to stars.dat or extrasolar.ssc.
Pair of brown dwarfs found
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The official press release is at http://cfa-www.harvard.edu/press/pr0424.html
and the discovery preprint is at http://cfa-www.harvard.edu/~kluhman/paper.pdf
They're members of the Chamaeleon I star forming region.
and the discovery preprint is at http://cfa-www.harvard.edu/~kluhman/paper.pdf
They're members of the Chamaeleon I star forming region.
Selden
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http://cfa-www.harvard.edu/~kluhman/paper.pdf.
Can't quickly spot a distance.
Spiff.
Code: Select all
Comp. R.A.(J2000) Dec (J2000)
A 11 01 19.218 -77 32 38.60
B 11 01 19.438 -77 32 37.36
Can't quickly spot a distance.
Spiff.
160 +/- 15 parsecs
Ref: Whittet etal. 1997, A&A, 327, 1194
briefly, see:
http://aa.springer.de/papers/7327003/2301194/small.htm
Ref: Whittet etal. 1997, A&A, 327, 1194
briefly, see:
http://aa.springer.de/papers/7327003/2301194/small.htm
Selden
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- Posts: 1386
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Evil Dr Ganymede wrote:I dunno... why couldn't this pair of dwarfs have formed separately and been captured into their distant orbit around eachother during a later encounter?
Is there any information on their orbital eccentricity? I would think that the higher the eccentricity, the more likely that one became bound to the other much later.
Of course, this might be a poor determination.....
...John...
"To make an apple pie from scratch, you must first create the universe..."
--Carl Sagan
--Carl Sagan