Sister blog of Physicists of the Caribbean. Shorter, more focused posts specialising in astronomy and data visualisation.
Thursday, 10 May 2018
Scanning a galaxy
And another one. To recap, this is a plot through an HI data cube, where instead of plotting a map of the brightness of the gas, the measured flux corresponds to the height of the line. Each line is a horizontal slice through the data at a single frequency channel, effectively a plot of flux as a function of right ascension (NOT a spectrum !). All I've done here is have each line reveal itself successively, adding a material to make the newly-revealed lines brighter and the older ones faded.
Next up will be to try and simultaneously animate both the appearance of the lines and their corresponding spectral channel, so that the entire surface will be constantly in motion.
Subscribe to:
Post Comments (Atom)
Nobody Ram Pressure Strips A Dwarf !
Very attentive readers may remember a paper from 2022 claiming, with considerable and extensive justification, to have detected a new class...
-
Of course you can prove a negative. In one sense this can be the easiest thing in the world : your theory predicts something which doesn...
-
In the last batch of simulations, we dropped a long gas stream into the gravitational potential of a cluster to see if it would get torn...
-
Why Philosophy Matters for Science : A Worked Example "Fox News host Chris Wallace pushed Republican presidential candidate to expand...
No comments:
Post a Comment