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Credit & Copyright: X-ray:
Andrew Wilson (UMCP)
et al.,
NASA,
CXC
Optical: DSS / IR: NASA, JPL-Caltech / Radio: NRAO, AUI, NSF
Explanation:
Better known as M106, bright
spiral galaxy
NGC 4258 is about 30 thousand light years across and
21 million light years away
toward the northern constellation
Canes Venatici.
The yellow and red hues in
this composite
image show the
galaxy's sweeping
spiral arms
as seen in visible and
infrared light.
But x-ray
and
radio data
(blue and purple) reveal two extra
spiral arms -- arms that don't align with the more familiar tracers
of stars, gas, and dust.
In fact,
an analysis
of the x-ray and radio data suggests
that the anamolous arms are composed of material heated
by shock waves.
Detected at radio wavelengths,
powerful jets originating in the
galaxy's core likely drive the shocks into the disk
of NGC 4258.
Optical: DSS / IR: NASA, JPL-Caltech / Radio: NRAO, AUI, NSF
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: M 106 - spiral galaxy - spiral arms - radio
Publications with words: M 106 - spiral galaxy - spiral arms - radio
See also:
- APOD: 2025 September 4 Á NGC 4565: Galaxy on Edge
- APOD: 2025 August 22 Á A Tale of Two Nebulae
- APOD: 2025 August 19 Á Giant Galaxies in Pavo
- APOD: 2025 August 18 Á NGC 1309: A Useful Spiral Galaxy
- APOD: 2025 July 4 Á NGC 6946 and NGC 6939
- APOD: 2025 June 30 Á NGC 4651: The Umbrella Galaxy
- APOD: 2025 June 19 Á NGC 3521: Galaxy in a Bubble