Not exact matches
How about cosmic microwave background radiation, time dilation
in supernovae light curves, the Hubble deep
field, the Sunyaev - Zel «dovich effect, the Integrated Sachs - Wolfe effect, the hom.ogeneity of stars and galaxies, etc, etc...
Working with NASA on its Wide -
Field Infrared Survey Telescope (WFIRST) mission, due to launch sometime after 2020 (see «Mapping the Dark,» page 47), Perlmutter will help choose between the different models by studying groups of
supernovae that lie farther out
in space than any yet studied, following the universe's expansion history back
in time.
But Michilli points out that
in order to drive such strong magnetic
fields, the
supernova remnant would have to be a million times brighter than even the brightest remnant
in the Milky Way, the Crab nebula (SN: 1/1/11, p. 11).
More common lower - energy cosmic rays — thought to emerge
in the aftermath of
supernova explosions
in the Milky Way — curve so much
in the galaxy's magnetic
field that they appear to come from all over the sky.
The circular rings
in the center - left of the image are
supernova remnants caught
in the strong magnetic
field of the galaxy's core.
Janka «is doing the leading work»
in this highly competitive
field, says
supernova pioneer Stanford Woosley of the University of California, Santa Cruz.
The stronger moving magnetic
fields produced
in supernova explosions could provide the energy for most other cosmic rays.
We find good agreement
in the regions of ove... ▽ More We derive an accurate mass distribution of the galaxy cluster MACS J1206.2 - 0847 (z = 0.439) from a combined weak - lensing distortion, magnification, and strong - lensing analysis of wide -
field Subaru BVRIz» imaging and our recent 16 - band Hubble Space Telescope observations taken as part of the Cluster Lensing And
Supernova survey with Hubble (CLASH) program.
With the advent of new wide -
field, high - cadence optical transient surveys, our understanding of the diversity of core - collapse
supernovae has grown tremendously
in the last decade.
This means they could predict when and where
in the
field the image of the
supernova would appear next.
Photographed about eight days after it exploded,
Supernova 1997ff (SN1997ff) was found by astronomers comparing the northern Hubble Deep
Field, a 10 - day observation of a tiny region of sky first explored by the Hubble Space Telescope
in 1995, with a follow - up observation
in 1997.
[Obviously, if they were any further away, or if the random
supernovas blew up too early to become part of the solar system's dust cloud, or were traveling too fast to be captured by what would become part of the solar system's dust cloud, or were thrown out too slow to get here
in time, or were formed but were inside another star gravity
field and never thrown back into space, even more dust would be lost
in space, but let's keep the problem easy.
GCRs are modulated by both solar magnetic
field, which is largely unpredictable
in strength except for generalities associated with 11 - year sunspot cycle and is also modulated by unpredictable events like nearby
supernovas, and by more predictable very very long slow changes
in intensity due to the solar system traversing spiral arms of our galaxy and wandering above and below the galactic plane
in cycles lasting tens and hundreds of millions of years.