HI Galactic Halo Cloud G19.4+6.3 (collage)

Minimum credit line: Image courtesy of NRAO/AUI and Yurii Pidopryhora, NRAO & Ohio University(for details, see Image Use Policy).

About this 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 collage shows one of such clouds (G19.4+6.3) as seen at its peak by the GBT in the larger Galactic halo context and its VLA HI column density map with two VLA sample spectra taken at the cloud's cores. The GBT image shows that the cloud is a part of a larger cloud-filament structure, while the VLA image reveals that the cloud has a "dense core - diffuse envelope" structure. The assymetry of the envelope might also suggest a sideway motion. It can be estimated that this cloud is about 8 kpc away from us and 900 pc above the Galactic plane. Its size is approximately 30 pc with core size of about 10 pc. This cloud contains 800 solar masses of hydrogen and the desity of its cores exceeds 20 atoms per cubic cm. The images are false-color with blue corresponding to the least and red -- to the most hydrogen density.

Investigator(s):  Liszt, H., Lockman, J., Rupen, M. (NRAO), Pidopryhora Y. (NRAO & Ohio U)

Alternate Resolutions Help

This image is available in the following downloadable versions:If you would like to obtain a higher resolution version of this image, please contact us.

For More Information

Technical Data

    Telescope VLA 
    Date of Observation 2004-07-03 
    Type of Observation Spectral Line Observations 
    Center of Image RA: 18:04:0.00, Dec: -8:58:0.00 (J2000)  
    Field of View 2.0000 x 6.0000 degrees  
    Technical Caption The resolutions: GBT image -- 9 arcmin, VLA (taken in D-array) -- 1 arcmin. GBT exposure 5 sec per 3 by 3 arcmin pixel, VLA -- a few hours. Cloud's peak column density is 4x10^+20 cm^-2 and the line's FWHM is 4.4 km/s, as measured from the VLA data.  

  • Astronomical database entries for HI cloud G19.4 6.3
    • Query SIMBAD for more HI cloud G19.4 6.3 data


To search the Image Gallery for other images of HI cloud G19.4 6.3, click the Submit button.
Object Name Show Results As:

To search the Image Gallery for similar images, click the Submit button.
Category Sub-Category Telescope Mode Show Results As:

For more search options, please use our Advanced Search form.