ubiquitous bright blue 1-12 pixel sources on darker 3D fractal web in five
2007.09.06 IR and visible light HUDF images, Nor Pirzkal, Sangeeta Malhotra,
James E Rhoads, Chun Xu, -- might be clusters of earliest hypernovae in recent
cosmological simulations: Rich Murray 2008.08.17 2009.01.20

ubiquitous bright blue 1-12 pixel sources on darker 3D fractal web in
five 2007.09.06 IR and visible light HUDF images, Nor Pirzkal,
Sangeeta Malhotra, James E Rhoads, Chun Xu, -- might be clusters of
earliest hypernovae in recent cosmological simulations: Rich Murray
2008.08.17
rmforall.blogspot.com/2008_08_01_archive.htm
Sunday, August 17, 2008
groups.yahoo.com/group/AstroDeep/25
groups.yahoo.com/group/rmforall/85

www.flickr.com/photos/rmforall/1349101458/in/photostream/

The 5 closeups are about 2.2x2.2 arc-seconds wide and high, about
70x70 pixels.
The HUDF is 315x315 arc-seconds, with N at top and E at left.
Each side has 10,500x10,500 pixels at 0.03 arc-second per pixel.

Click on All Sizes and select Original to view the highest resolution
image of 3022x2496 pixels, which can be also be conveniently seen
directly at their Zoomable image:

www.spacetelescope.org/images/html/zoomable/heic0714a.html

Notable in the deep background of the five closeups are ubiquitous
bright blue sources, presumably extremely hot ultraviolet before
redshifting, 1 to a dozen or so pixels, as single or short lines of
spots, and a few irregular tiny blobs, probably, as predicted in many
recent simulations, the earliest massive, short-lived hypernovae, GRBs
with jets at various angles to our line of sight, expanding bubbles,
earliest molecular and dust clouds with light echoes and bursts of
star formation, and first small dwarf galaxies, always associated with
a subtle darker 3D random fractal mesh of filaments of H and He atomic
gases.

As a scientific layman, I am grateful for specific cogent, civil
feedback, based on the details readily visible in images in the public
domain.

www.spacetelescope.org/images/html/heic0714a.html

Hubble and Spitzer Uncover Smallest Galaxy Building Blocks

notable bright blue tiny sources on darker 3D fractal web in HUDF VLT
ESO 28 images from 506 galaxies, z about 6 , RJ Bouwens, GD
Illingworth, JP Blakeslee, M Franx 2008.02.04 draft 36 page:
Rich Murray 2008.08.17
rmforall.blogspot.com/2008_08_01_archive.htm
Sunday, August 17, 2008
groups.yahoo.com/group/AstroDeep/26
groups.yahoo.com/group/rmforall/86

bright blue 1-4 pixel sources on darker 3D fractal web in IR and
visible light HUDF images -- might be the clusters of earliest
hypernovae in the Naoki Yoshida and Lars Hernquist simulation:
Rich Murray 2008.07.31
rmforall.blogspot.com/2008_07_01_archive.htm
Thursday, July 31, 2008
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groups.yahoo.com/group/rmforall/84

Rich Murray, MA Room For All rmforall@... 505-501-2298
1943 Otowi Road, Santa Fe, New Mexico 87505
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I show dozens of these lovely 20-120 MB images with my computer and an Epson
VX30 projector Tuesdays, 7:15 pm, at LaFarge Library, Llano Street, Santa Fe,
New Mexico 87505, just north of Siringo Road and south of St. Michael's Drive.

You are welcome to visit me and share your comments as I share these images at
home on a 4X8 foot screen.

Anyone may view and download for free 91 images, presenting the HUDF in eight 20
MB pieces at rmforall at www.FlickR.com -- #86 is about 20% of the HUDF in their
red and blue colors, as leaving out the green greatly simplifies interpreting
the overlapping layers of transparent fractal webs of gas with a wide range of
sizes of rather distant sources, beyond z = 5.