Past
radio observations revealed that gas is circling around the star to form a disk and we see the disk edge - on.
Not exact matches
ESA's Mars Express spacecraft orbiting overhead was also watching Schiaparelli's
radio signal, but a preliminary analysis of those
observations has proved inconclusive beyond
revealing the same sudden loss of signal.
The latest ALMA
observations, however,
reveal long filaments of cold molecular gas condensing around the outer edges of the
radio bubbles.
Also, the
radio observation results of molecular line emission of methanol
revealed in vivid detail an hourglass structure created by gas outflows spreading outward while thrusting the ambient gas cloud away.
Those
observations, published today in Nature,
reveal that the location of the bursts coincides with a faint, remote galaxy that also hosts a faint, persistent source of
radio waves.
The new VLA
observations revealed previously undetected regions where shocks accelerated subatomic particles, causing
radio emission.
Extremely sharp
observations of the event Swift J1644 +57 with the
radio telescope network EVN (European VLBI Network) have
revealed a remarkably compact jet, shown here in yellow.
The record - sharp
observations reveal a compact and surprisingly slowly moving source of
radio waves, with details published in a paper in the journal Monthly Notices of the Royal Astronomical Society.
A month later, follow - up
observations with the Lovell
radio telescope in Cheshire, UK,
revealed periodic variations in the pulsar's signals, indicating the existence of an orbiting companion with the mass of a planet.
Observations with the Very Large Array near Socorro, New Mexico,
revealed two objects whose
radio spectra resemble those of other black hole systems located outside of star clusters.
Those
observations reveal that the location of the bursts coincides with a faint, remote galaxy that also hosts a persistent source of
radio waves.
In addition to detecting the bright bursts from FRB 121102, the VLA
observations also
revealed an ongoing, persistent source of weaker
radio emission in the same region.
Observations of Comet Hyakutake with the National Science Foundation's millimeter - wave
radio telescope in Arizona have
revealed new information about our Solar System's original material, including the first detection of the Carbonyl Sulfide (OCS) molecule in a comet.
Observations of Comet Hyakutake with the National Science Foundation's millimeter - wave
radio telescope in Arizona have
revealed new information about our Solar System's original material, including the first detection of the Carbonyl Sulfide molecule in a comet.
The
radio observations have
revealed a size of the fireball, unobtainable by any other technique, thereby enabling astronomers to learn about inner workings of such objects,» said Shri Kulkarni, professor of astronomy at the California Institute of Technology (Caltech).
Hallinan is planning continued
radio observations over the next year or two, because this
radio emission — which will be around long after all of the other wavelengths have faded — is the most important diagnostic of the energetics and environment of the explosion, and may
reveal how much energy was in the explosion, how much mass was ejected, if a jet actually appeared, and if the merger produced conditions that will influence future star formation, among other questions.