... A total of 326 GMCs in the mass range 104-107 M т?? are identified; their cumulative mass distribution is found to be proportional to M -2.34, in agreement with earlier studies. ...
... normalized by dividing by the values measured with the 11 pixels height. a) Results for m = 107 of E140M around 1380 е. b) Results for m = 104 around 1960 е. c) Results for m = 346 of E230H around 2230 е. a) m=107, E140M, 1380е b) m=104, E230M, 1960е c) m ...
... Similarly, in the Local Group dwarf elliptical galaxy NGC 205, MBH < 3.8 в 104M [40 ... a more massive see d BH with MBH 104 - 106 M from a collapsing metal-free gas cloud ...
... an upper limit to the cluster mass of 7(104 ) M within a radius of 0.23 pc; we also ... observations to estimate a total cluster mass ( 104M ) and radius (0.2 pc) to ...
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Ссылки http://www.stsci.edu/science/preprints/prep1563/prep1563.pdf -- 1758.0 Кб -- 26.11.2002 Похожие документы
... C h a r a c t e r is t ic H a lo M a s s S c a le s (masses at redshift z=10) · Jeans Mass · H2 cooling · HI cooling · Photo-heating 104M Tvir=20 K Tvir=102 K Tvir=104 K Tvir=2x105 K z=20 z=17 z=9 z=5 1 05 M 1 08 M 1 01 0 M JWST: 1nJy M* 107 M or Mbh 105 ...
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Ссылки http://www.stsci.edu/institute/conference/jwst2007/Presentations_Posters/haiman_talk.pdf -- 1107.8 Кб -- 20.03.2012 Похожие документы
... M for Gl 105A (Henry & McCarthy _ 1993), we compute that a VLM companion would induce peak-to-peak velocity variations of D1.75 ] 104M sin i vlm (m s~1), where M is the mass of the VLM companion (in vlmis the inclination of the orbit relative to solar ...