Credit: X-Ray: J. Grindlay
(CfA) et al.,
CXO,
NASA
Optical: W. Keel (U. Alabama Tuscaloosa) et al., 1.5-m Telescope, CTIO
Explanation:
A deep optical image (left)
of 47 Tucanae shows an ancient
globular star cluster so dense and crowded that individual stars
can not be distinguished in its closely packed core.
An
x-ray image of its central regions (inset right) from the
Chandra
Observatory reveals a wealth of x-ray stars hidden there.
Color-coded by energy, low energies are red, medium green,
and high energy cosmic
x-ray sources are blue, while
whitish sources are bright across the x-ray energy bands.
The x-ray stars here are double stars or "compact"
binary star systems.
They are so called because one of the pair of stellar companions is
a normal star and the other a compact object --
a white dwarf,
neutron star,
or possibly a black hole.
Chandra's
x-ray vision detects the presence of
an unexpectedly large number of these exotic star systems
within 47 Tucanae, but it also indicates the apparent
absence of a large central black hole.
The finding suggests that compact binary star systems of
47 Tucanae
may be ejected from the cluster before coalescing
to form a large black hole at its core.
Optical: W. Keel (U. Alabama Tuscaloosa) et al., 1.5-m Telescope, CTIO
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Publikacii s klyuchevymi slovami:
neitronnye zvezdy - globular cluster - dvoinye zvezdy - rentgenovskoe izluchenie - Pul'sar - pulsar - neutron star - binary star - Sharovoe skoplenie
Publikacii so slovami: neitronnye zvezdy - globular cluster - dvoinye zvezdy - rentgenovskoe izluchenie - Pul'sar - pulsar - neutron star - binary star - Sharovoe skoplenie | |
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