Longitude and Latitude velocity plots
Longitude-velocity and Latitude-velocity plots
Observing velocity profiles of the HI lines at different longitudes, we can derive a diagram in which the intensity distribution is mapped in the position-velocity space, namely in the l-vr plane. This is called a longitude-velocity diagram. The LV diagram is used for studying the rotation characteristics of the galactic disk as well as to derive the spiral structure.[Y.Sofue, Galactic Radio Astronomy].
The HI spectrums that I observed give us the information needed to construct the l-v diagrams.
Data
I'll write more about the "observation" part in a later post. But for now, just take it that we get the velocities and the corresponding latitudes from this data.
Longitude-velocity plots
l-v plot at latitude b=0 |
l-v plot using data at b=0 latitude |
The arm near the 0 km/s mark is the Local arm, while the -50 km/s is the Perseus and the one nearing the end around -100 km/s is the Outer arm. The upper triangle contains the Saggitarius-Carina and Scutum-Centaurus arm.
Gas with positive velocities represents those inside the solar circle (R < Ro), and negative velocities are those outside the solar circle R > Ro. The solar circle is the circle with the radius equalling the distance of the solar system to the center of the galaxy. (Ro=8.05 Kpc).
Have a look at Koo et.al (2017) paper. They used different tracers to do the same. Unlike me they weren't limited to longitude 0-220 degrees, they had the whole sky to work on. Keep in mind they use the [-180:180] layout instead of the [0:360] layout for the longitude-velocity plots.[Link]
Latitude-velocity plots
In a similar way, we can obtain a latitude-velocity diagram by scanning in the direction of the latitude (perpendicular to the galactic plane). A b-v diagram is used for obtaining information about the disk thickness and distribution of the gas in the z-direction. It is often used for studying the warping of the outer galactic disk.[Y.Sofue, Galactic Radio Astronomy].
For constructing the b-v plots I observed at two different longitudes l=90 and l=120 degrees in the latitude range -20<b<20 degrees.
l=120 degrees
Local, Perseus and the Outer arm are visible |
Nice 👍🏻
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