The Spatial Extent of Line-Emitting Regions in the Cloverleaf

Details The Spatial Extent of Line-Emitting Regions in the Cloverleaf The Spatial Extent of Line-Emitting Regions in the Cloverleaf

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aas...20514308h&link_type=abstract

American Astronomical Society Meeting 205, #143.08; Bulletin of the American Astronomical Society, Vol. 36, p.1585

Astronomy and Astrophysics

Astronomy

Scientific paper

The Cloverleaf QSO (H1413+1143) is a four-component gravitationally-lensed broad absorption line (BAL) QSO with an emission redshift of z=2.55. HST broad-band imaging shows the four components to be unresolved and separated by about 1 arcsec. These broad-band images primarily show H1413+1143's compact continuum-emitting region. However, by imaging in the line-emitting regions we can hope to use the natural lens present in the Cloverleaf to study the sizes of these more spatially-extended regions. Here we report on the results of such observations.

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