scholarly journals Diagnosing the Outflow from the SGR 1806-20 Giant Flare with Radio Observations

2005 ◽  
Author(s):  
J Granot
Keyword(s):  
Radio Observations ◽  
Giant Flare

Multi wavelenght radio observations of Cygnus X-3 during the giant flare of May-June 2006

2008 ◽  
Author(s):  
Sabyasachi Pal ◽  
C. H. Ishwara-Chandra ◽  
A. Pramesh Rao ◽  
Sandip K. Chakrabarti ◽  
Archan S. Majumdar
Keyword(s):  
Radio Observations ◽  
Giant Flare

scholarly journals Diagnosing the Outflow from the SGR 1806−20 Giant Flare with Radio Observations

2006 ◽  
Vol 638 (1) ◽  
pp. 391-396 ◽  
Author(s):  
J. Granot ◽  
E. Ramirez‐Ruiz ◽  
G. B. Taylor ◽  
D. Eichler ◽  
Y. E. Lyubarsky ◽  
...  
Keyword(s):  
Radio Observations ◽  
Giant Flare

scholarly journals Multi frequency radio observations of Cygnus X-3 during the giant flare of May-June 2006

2009 ◽  
Author(s):  
Sabyasachi Pal ◽  
Isvwara Chandra ◽  
A. Pramesh Rao
Keyword(s):  
Radio Observations ◽  
Giant Flare

Low frequency radio observations: critical in revealing inhomogeneous shock structures

2019 ◽  
Author(s):  
Poonam Chandra ◽  
A. J. Nayana ◽  
Claes-Ingvar Bjornsson ◽  
Peter Lundqvist ◽  
Alak K. Ray
Keyword(s):  
Low Frequency ◽  
Radio Observations

scholarly journals Rapid spectral variability of a giant flare from a magnetar in NGC 253

Nature ◽  
2021 ◽  
Vol 589 (7841) ◽  
pp. 207-210 ◽  
Author(s):  
O. J. Roberts ◽  
P. Veres ◽  
M. G. Baring ◽  
M. S. Briggs ◽  
C. Kouveliotou ◽  
...  
Keyword(s):  
Spectral Variability ◽  
Giant Flare

scholarly journals Physical Conditions in the Compact Planetary Nebula Sw St 1

1983 ◽  
Vol 103 ◽  
pp. 520-520
Author(s):  
M. Cohen ◽  
D.R. Flower ◽  
A. Goharji
Keyword(s):  
Electron Density ◽  
Planetary Nebula ◽  
Emission Measure ◽  
Emission Feature ◽  
Radio Observations ◽  
Physical Conditions ◽  
Infra Red ◽  
High Emission

Sw St 1 is a compact and possibly young planetary nebula which has been recently observed at infra red (Aitken et al., 1979) and radio (Kwok et al., 1981) wavelengths. In the 8-13 μm region, a silicate emission feature is observed, suggesting that the nebular envelope is oxygen rich. The high emission measure determined from the radio observations implies a large value for the electron density.

Radio Observations of Interstellar Formaldehyde

1969 ◽  
Vol 1 (6) ◽  
pp. 282-283 ◽  
Author(s):  
J. B. Whiteoak ◽  
F. F. Gardner
Keyword(s):  
Transition Frequency ◽  
Radio Observations

The 111–110 transition (frequency 4829.65 MHz) of formaldehyde (CH2O) has been recently observed in absorption against a number of continuum sources by Snyder et al. with the Green Bank 140-ft telescope.

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