Radio recombination line (H92alpha) observations of SGR E

Details Radio recombination line (H92alpha) observations of SGR E Radio recombination line (H92alpha) observations of SGR E

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.280.1110c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 280, Issue 4, pp. 1110-1120.

Astronomy and Astrophysics

Astronomy

9

Hii Regions, Ism: Individual: Sgr E, Galaxy: Centre, Radio Continuum: Ism, Radio Lines: Ism

Scientific paper

Observations of radio recombination line (H92alpha) and 8.3-GHz continuum emission from several probable thermal sources in the Galactic Centre HII complex Sgr E have been made using the Very Large Array. Line emission has been detected from seven of these sources, confirming their thermal nature and also locating them in a single kinematical entity moving with nu_LSR~=-205 km s^-1. The continuum sources are well resolved by the 8-arcsec beam, and several have complex structure including shells, arcs and cores. One source (G 358.6+0.06) has no significant H92alpha flux, despite its relatively bright continuum and flat spectrum. Further observations will be needed to determine whether or not this interesting source is actually thermal.

Affiliated with

Also associated with

No associations

Rating

Radio recombination line (H92alpha) observations of SGR E does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radio recombination line (H92alpha) observations of SGR E, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radio recombination line (H92alpha) observations of SGR E will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1301569