This Document Contains the following:
1) Record all Distant sample measurements taken (below), 12_CO single
pointing
observations, maps, 13_CO single pointings, 13_CO maps.
2) Record all Distant Sample CO J=1-0 measurements from the literature
(Finish in June) giving apertures and fluxes.
3) Display the literature CO 1-0 data for the Nearby sample.
4) Add in Harriet's High J Observations.
5) Re-reduce the SEST runs and display.
6) Re-reduce the NRAO runs and display.
7) More CSO observations from Harriet.
8) Future SEST and NRAO data.
ALL OBSERVED SINGLE DISH CO 1-0 DATA
------------------------------------
NRAO Run SEST I
SEST II Lit. Refs
------------------------------------------------------------------------------
NGC_0278
1,2,3,4,5
NGC_0520
3,6,7,8
NGC_0693
obs'ed 3,9
NGC_0695
3,10
UGC_01449 mapped
11?
MCG-03-06-01 mapped
obs'ed
NGC_0986
mapped 2,6,8,12,13-16
NGC_1022
obs'ed 13
NGC_1052
UGC_02238
NGC_1155 mapped
NGC_1156
NGC_1222
UGC_02519 mapped
NGC_1266
NGC_1317
NGC_1326
NGC_1385
obs'ed 12,13 obs'ed
13
UGC_02855
NGC_1482
NGC_1546
obs'ed 12, 13
NGC_1569
NGC_2388
ESO317-G023
mapped
IRASF10565+2 obs'ed
NGC_3583
NGC_3620
mapped
obs'ed 12, 13
NGC_3683
NGC_3705 obs'ed
NGC_3885
mapped
NGC_3949 mapped
NGC_4027
NGC_4102
NGC_4194
NGC_4418
NGC_4490
NGC_4519 mapped
NGC_4691
NGC_4713
IC__3908 mappedNGC_6286
IC__4662
obs'ed
NGC_6753
mapped,13
obs'ed 13
NGC_6821 obs'ed
obs'ed
NGC_6958
obs'ed
obs'ed
NGC_7218 obs'ed
NGC_7418 mapped
mapped
IC__5325
mapped
IRASF23365+3
NGC_7771
MRK_0331
NGC 6744
obs'ed
mapped
-----
NGC 2397
mapped
mapped, o'ed 13
NGC 4800 mapped
IC__0860
IC__0883
NGC_5433 obs'ed
NGC_5713
NGC_5786
obs'ed
NGC_5866
CGCG1510.8+0IC 4664
obs'ed
NGC_5962
IC__4595
mapped
1) 1997ApJ...485..552M MAIOLINO, R., R...
2) 1996A&AS..115..439E ELFHAG, T., BOO...
3) 1995ApJS...98..219Y YOUNG, J. S., X...
4) 1993A&AS...97..887B BRAINE, J., COM...
5) 1989ApJ...342..735H HECKMAN, T. M.,...
This is a preliminary (not final!!) list.
I_CO K km/s CII (W/cm2)
Galaxy
--------------------------------------
9.0
0.2978e-18 N7771
9.2
0.1478e-18 Mk331
7.9
0.7281e-18 N278
16.6
0.2828e-18 N520
4.8
0.2035e-18 N695
5.3
0.1870e-18 N1022
6.0
0.2351e-18 U2238
14.5
0.5237e-18 U2855
11.0
0.6392e-18 N1482
7.3
1.94e-19 I5325
26.1
1.94e-19 N3620
3.88
1.4e-19 N3885
6.5
1.31e-19 N5786
12.8
2.22e-19 N6753
7.72
1.e-19 E317C
12.42
2.47e-19 I4595
10.51
1.34e-19 N7418
3.4
2.8e-20 CGCG1
1.1
3e-20 I0860
4.2
9.54e-20 I0883
10.1
1.89e-19 N3583
7.6
4.07e-19 N3683
10.0
3.2e-19 N4102
4.1
2.01e-19 N4194
4.7
3.e-20 N4418
6.3
4.95e-19 N4490
8.22
2.87e-19 N4691
6.0
4.3e-19 N5713
2.3
6.84e-20 N5866
7.8
2.37e-19 N5962
Figure from Lord et al. 1999, showing the ISO C+ [W/m^2] and groundbased CO (J=1-0) [K km/s] fluxes, normalized to the FIR emission (IRAS data), for galaxies from the Key Project on Normal Galaxies (Helou et al. 1999; open circles). Also shown for comparison are the starburst (asterisks) and Ultra-Luminous Infrared Galaxy (ULIRG; filled circles) samples of Luhman et al. (1998, 1999), and the low-luminosity Virgo spirals (open squares) studied by Smith and Madden (1997). Note the Key Project sample spans the full range of observed parameters from quiescent to very active systems, including three objects of moderate luminosity and redshift which may be used as ULIRG analogs.
Predicted flux ratios from PDR models for the gas density n, and
interstellar radiation field intensity G_0 from Stacey et al. 1991 are
superposed as the grid of curves. There is some degeneracy in separating
various values of n, but G_0 clearly increases from right to left.
Normal and starburst galaxies typically fall in the range of 10^2>n>10^4
and 10^2