05.06.2013 Views

The Caldwell Objects

The Caldwell Objects

The Caldwell Objects

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

55<br />

the companion would have to be located about<br />

4.5 solar radii from the central star to account for<br />

the misalignment of the inner ellipsoids.<br />

A recent discovery also revealed a dim inner pair<br />

of condensations that resembles the well-known<br />

outer pair, with one knot on either side of the<br />

central star. <strong>The</strong> condensation pairs may have<br />

originated in separate shells of ejected matter that<br />

have since been pushed outward by the central<br />

star's ultraviolet radiation or particulate winds.<br />

<strong>The</strong> International Ultraviolet Explorer satellite<br />

found no evidence of light-scattering<br />

220<br />

dust particles in NGC 7009.<br />

In April 1996 the Hubble Space Telescope imaged<br />

NGC 7009, giving astronomers an unprecedented<br />

look at this complex planetary nebula. An<br />

enhanced color version of this image (a blackand-white<br />

version is shown below) shows a<br />

central star trapped in the cavity of a pale blue<br />

chrysalis of gas. Large hollow lobes of yellow gas<br />

extend from this chrysalis, making the inner<br />

nebula look like some sort of psychedelic sushi.<br />

<strong>The</strong> green outer envelope (the star's former outer<br />

layers) appears some-<br />

what boxy and multidimensional,<br />

like a time-lapse<br />

exposure of an open beer<br />

barrel rolling in a circle.<br />

Thin green jets extend along<br />

the nebula's major axis and<br />

end in bright blood-red<br />

knots, as if the jets were<br />

recently cauterized veins. If<br />

the nebula is 1,400 lightyears<br />

distant, these knots lie<br />

0.15 light-year from the<br />

central star. Despite its<br />

visual com<br />

plexity, the HST image is giving astronomers a<br />

better understanding of the mysterious processes<br />

that transform a low-mass star like our Sun into a<br />

white dwarf. A computer model based on the<br />

HST data indicates that NGC 7009's progenitor<br />

star first expelled one solar mass of gas, which<br />

now constitutes the "barrel." This gas confines<br />

stellar winds flowing from the central star. <strong>The</strong><br />

confined gases slide along the walls of the<br />

barrel's cavity until they converge at its tips. As<br />

Bruce Balick (University of Washington)<br />

explains, "Each ansa [terminal knot] is joined to<br />

the tips of the cavity by a long greenish jet of<br />

material, much like the hot gases that<br />

follow a bullet from the barrel of a rifle __ <strong>The</strong><br />

tips act somewhat like a nozzle that form gas<br />

Deep-Sky Companions: <strong>The</strong> <strong>Caldwell</strong> <strong>Objects</strong>

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!