none103siWe present the first detection of carbon radio recombination line absorption along the line of sight to Cygnus A. The observations were carried out with the Low Frequency Array in the 33-57MHz range. These low-frequency radio observations provide us with a new line of sight to study the diffuse, neutral gas in our Galaxy. To our knowledge this is the first time that foreground Milky Way recombination line absorption has been observed against a bright extragalactic background source. By stacking 48 carbon α lines in the observed frequency range we detect carbon absorption with a signal-to-noise ratio of about 5. The average carbon absorption has a peak optical depth of 2 × 10-4, a line width of 10 km s-1 and a velocity of +4 kms-1 w...
We present the first detection of carbon radio recombination line absorption along the line of sight...
Carbon radio recombination lines (RRLs) at low frequencies (≲ 500 MHz) trace the cold, diffuse phase...
Carbon radio recombination lines (RRLs) at low frequencies ( 72 500 MHz) trace the cold, diffuse pha...
We present the first detection of carbon radio recombination line absorption along the line of sight...
We present the first detection of carbon radio recombination line absorption along the line of sight...
Carbon radio recombination lines (RRLs) at low frequencies (≲ 500 MHz) trace the cold, diffuse phase...
Carbon radio recombination lines (RRLs) at low frequencies ( 72 500 MHz) trace the cold, diffuse pha...
We present the first detection of carbon radio recombination line absorption along the line of sight...
We present the first detection of carbon radio recombination line absorption along the line of sight...
Carbon radio recombination lines (RRLs) at low frequencies (≲ 500 MHz) trace the cold, diffuse phase...
Carbon radio recombination lines (RRLs) at low frequencies ( 72 500 MHz) trace the cold, diffuse pha...