March 14, 1997
Hi All--
Here's what I think our plan should be for the March FCRAO observing
run.
Our goal is to make a plot like this:
Only, our axes will be straighter, and real data will be involved. Paola
and I guessed about which molecules will trace which line width/size regimes,
but we should be close.
The first core we'll attack is TMC-1C (see coordinate table at
end of this document). We already have a good NH3 map, and an
OH map. The OH probably traces an even lower density (larger scale) than
the C18O, but I didn't draw it in my sketch (sorry!). In the
"Maps" section of the notebook, you'll find the map of TMC-1C
in N2H+ that Paola made at FCRAO. It was made as a
single footprint, observed for 15 minutes, and Paola thinks we should just
re-do it, for the sake of convenience & consistency. In the "Proposals"
section, you'll find maps of TMC-1C in OH and NH3, as a figure
in the IRAM proposal.
After TMC-1C, I think we should move on to either L1512 or L1251A.
L1512 has the advantage of being small and boringly-shaped (round), and
Paola's already made a Nyquist sampled N2H+ map of
it (see the "Maps" section). L1251A is larger, and we already
have N2H+, NH3, and C18O maps
of it. I guess we should go for L1512 first, since this is officially "Taurus"
time, and we can save L1251 for time in April?
With all that information in-hand, I think we should do the following
for each core we observe:
Move on to the next core and do essentially the same thing, taking care not to duplicate tracers already observed (see above).
The N2H+ frequency-switching scheme for a 10 MHz BW is shown here.
Coordinates and offsets to the peak position for all the sources
are given in Paola's N2H+ summary table, N2Hplusmaps.ps.
Be careful to use the "TMC-1C" entry, and none of it's variants.
Same goes for L1251A. The LSR velocities are 5.2 km/s for TMC-1C,
~4 km/s for L1512, and -4.3 km/s for L1251A.
As mentioned above, I've put maps of these sources in the "sources" section of the notebook.