HI Galactic Halo Cloud G27.0+6.3 (VLA image)

Since 2002 hundreds of HI (neutral hydrogen) clouds have been discovered with the help of the new unique NRAO instrument -- 100 m Green Bank Telescope (GBT). These clouds are a completely new class of objects presenting a previously unknown phenomenon of the interstellar matter physics. Several brightest of them have been observed with another NRAO instrument, Very Large Array (VLA) which provides better angular resolution. This image shows one of such cloud's (G27.0+6.3) VLA HI column density map. It reveals that the cloud has a "dense core - diffuse envelope" structure. The assymetry of the envelope might also suggest a downward motion. It can be estimated that this cloud is about 7.5 kpc away from us and 850 pc above the Galactic plane. Its size is approximately 20 pc with core size of about 7 pc. This cloud contains 500 solar masses of hydrogen and the density of its core exceeds 20 atoms per cubic cm. The image is a false-color one with blue corresponding to the least and red -- to the most hydrogen density.

The image resolution (taken in VLA D-array) is 1 arcmin, exposure is a few hours. Cloud's peak column density is 3.5x10^+20 cm^-2 and the line's FWHM is 4.8 km/s, as measured from the VLA data. Distance estimated assuming the cloud resides at the tangent point.

Legacy Astronomical Images

NRAO/AUI/NSF does not hold full copyright for this image. Contact the archivist for details.

Legacy Astronomical Image

HI cloud G27.0+6.3

Yurii Pidopryhora, NRAO & Ohio University

H. Liszt, J. Lockman, M. Rupen, Y. Pidopryhora

Very Large Array (VLA)

2004-07-10

spectral line

RA 18:18:0.000, Dec: -2:15:0.000 (J2000)

0.666667 x 0.500000 degrees

Contact the archivist for a high resolution tif of this image.

Galactic Sources Series

Galactic Halo Unit