Educação matemática pela arte
Gusmão, Lucimar Donizete
2013-08-28
Search results
15 records were found.
Comment: 5 pages, 3 figures, 2 tables, accepted in PASJ 50, Feb
Comment: 42 pages, 16 figures, ApJ in press, version with high resolution
figures is available via
http://www.nro.nao.ac.jp/~kmuraoka/m83paper/m83aste-otf.pdf
Comment: 12 pages, 1 table, 10 figures, accepted for publication in PASJ
Comment: 22 pages with 9 figures, Latex, accepted to PASJ
Comment: 39 pages, 7 figures, 4 tables. Accepted for publication in The
Astronomical Journal
Comment: 33 pages, 4 figures, 4 tables, accepted for publication in AJ
Comment: 18 pages, 4 figures, accepted for publication in ApJ
Comment: 13 pages, 11 figures, PASJ in press, version with high resolution
figures is available via http://www.nro.nao.ac.jp/~z5001km/m83-aste.pdf
Lyman-alpha emitters are thought to be young, low-mass galaxies with ages of
~10^8 yr. An overdensity of them in one region of the sky (the SSA 22 field)
traces out a filamentary structure in the early Universe at a redshift of z =
3.1 (equivalent to 15 per cent of the age of the Universe) and is believed to
mark a forming protocluster. Galaxies that are bright at (sub)millimetre
wavelengths are undergoing violent episodes of star formation, and there is
evidence that they are preferentially associated with high-redshift radio
galaxies, so the question of whether they are also associated with the most
significant large-scale structure growing at high redshift (as outlined by
Lyman-alpha emitters) naturally arises. Here we report an imaging survey of
1,100-um emission in the SSA 22 region. We find an enhancement of submillimetre
galax...


