Distances from time delays Water-maser proper-motions by VLBI
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Transcript of Distances from time delays Water-maser proper-motions by VLBI
Distances from time delays
Water-maser proper-motions by VLBI
Appears like the DawnFair as the MoonBright as the Sun
Majestic as the Stars
by Nari Jeong 2007. 7. 19
Distances from time delays
< Fundamental thinking >Astrophysical source’s light output changes
with time-> we can estimate its distance!!
The ring around Supernova 1987A
< Fact >IUE -> narrow emission lines from highly ionized
atoms in the spectrum of the supernova.
< Reason >Lines arise from radiation that has been
reprocessed bymaterial at some distance from the supernova.
< How to estimate distance >
Supernova : 52±3kpc
Gravitational lens time delays
< Fact >Large scales!! -> Gravitationally-lensed quasars.< Reason >Light passes a massive body -> path is bent by gravity.< How to estimate distance >The first term :
The second term : General-relativistic time dilation <- distortion of space-tim
e in the presence of a gravitational field
< Fact >Quasar has -> two images
< Reason >Different mass models would produce very different arrangements on the sky the multiple image.
< Kind >1. Multiple-image gravitational lens2. Luminous arc3. Radio ring4. Microlensing
< Q2237+0305, Einstein Cross >
Water-maser proper-motions by VLBI
Large distances!! - Bright enough to be readily detectable- Measure very small change = > H2O maser spots ( occur : active star formation )
VLBI ( very long baseline interferometry )
< Greenhill et at (1993) >H2O maser in M33 at two epochs separated by t = 479 days.Point out : large number of uncertainties
< Greenhill et al (1981) >Application of such a model to a Milky Way H2O maser Source.
< Miyoshi et al (1995) >VLBI observation : core of the nearby spiral galaxy NGC 4258.Distribution of H2O maser spots with a remarkably simple geometry.
< Figure 7.3 >Center – rotation as r^-1/2 – Keplerian mationMiddle – linearly – a single circular orbitEnd – similar center – disk’s inner edge=> Centripetally accelerated by the central mass
< Greenhill et al (1995) >Projected close to the center of the disk drift