ChanPlaNS

ChanPlaNS XVP Sample

To complete ChanPlaNS, we have requested an X-ray Visionary Program (XVP) through the Chandra X-ray Center Cycle 15 Call for Proposals. The 60 targets requested for the XVP comprise the remaining unobserved PNe in our volume-limited sample and, if awarded, would be acquired over the three cycles (15, 16, and 17).

Basic information and images of the XVP sample is provided in the following table.

ImageObjectNH
(1021cm-2)
D
(kpc)
Rneb
(pc)
Tstar
(kK)
Log L
(Lsun)
Binary?
NGC 6567
PN G011.7-00.6
2.811.680.03603.35nd
NGC 6537
PN G010.0+00.7
7.1920.052503.30nd
NGC 5882
PN G327.8+10.0
1.351.70.06683.52nd
NGC 6572
PN G034.6+11.8
1.101.860.06693.72u
NGC 3211
PN G286.3-04.8
1.101.910.071622.76nd
NGC 2792
PN G265.7+04.1
2.022.020.081263.18nd
IC 4642
PN G334.3-09.3
1.281.710.091133.22nd
NGC 6818
PN G025.8-17.9
1.281.640.11603.05w
NGC 6905
PN G061.4-09.5
0.761.580.151413.71u
NGC 2440
PN G234.8+02.4
1.561.90.182083.32nd
NGC 6563
PN G358.5-07.3
0.341.670.21232.34nd
NGC 2610
PN G239.6+13.9
0.011.720.21423.06w
SuWt 2
PN G311.0+02.4
1.911.50.221152.30c
K 1-27
PN G286.8-29.5
0.241.70.221052.68w
NGC 4071
PN G298.3-04.8
1.911.770.281302.17nd
Abell 59
PN G053.3+03.0
6.831.540.321022.09nd
Abell 46
PN G055.4+16.0
0.791.70.37662.80c
Abell 36
PN G318.4+41.4
0.140.450.421133.43n?
DS 2
PN G335.5+12.4
1.1010.46903.76n
NGC 5189
PN G307.2-03.4
1.811.440.461353.86y?
K 2-1
PN G173.7-05.8
2.201.50.481132.63nd
Wray 17-31
PN G277.7-03.5
1.211.40.491202.19nd
Abell 71
PN G084.9+04.4
3.761.330.511232.37nd
Abell 80
PN G102.8-05.0
1.911.520.521231.79nd
Abell 78
PN G081.2-14.9
0.271.850.521103.97n?
Abell 84
PN G112.9-10.2
1.311.680.531001.94nd
Abell 62
PN G047.1-04.2
0.691.380.54981.98nd
Abell 39
PN G047.0+42.4
0.101.40.591172.82n?
HaTr 7
PN G332.5-16.9
0.271.380.611003.04n
K 1-22
PN G283.6+25.3
0.241.330.621152.30w
Abell 61
PN G077.6+14.7
0.241.310.64881.73nd
Abell 34
PN G248.7+29.5
0.201.030.71982.05o?
PHR1432-6138
PN G314.5-01.0
1.311.190.711001.55nd
RCW 69
PN G302.1+00.3
2.631.30.731452.43nd
Jones 1
PN G104.2-29.6
0.440.90.741502.59n
MWP 1
PN G080.3-10.4
0.100.50.781633.30n
Lo 1
PN G255.3-59.6
0.010.760.781202.47n
Abell 13
PN G204.0-08.5
2.741.930.791131.99nd
Abell 24
PN G217.1+14.7
0.310.830.831371.90o
EGB 1
PN G124.0+10.7
1.140.650.871472.37n
Abell 21
PN G205.1+14.2
0.200.540.891362.04n
Abell 45
PN G020.2-00.6
4.021.320.931802.02nd
Abell 7
PN G215.5-30.8
0.100.511.01991.80w
Sh 2-78
PN G046.8+03.8
2.840.641.011121.88nd
EGB 6
PN G221.5+46.3
0.240.591.031101.86w
JnEr 1
PN G164.8+31.1
0.101.151.061162.02n
PuWe 1
PN G158.9+17.8
0.550.371.091091.70u
IsWe 1
PN G149.7-03.3
0.890.621.111001.74nd
Abell 31
PN G219.1+31.2
0.200.481.18941.69w
K 2-2
PN G204.1+04.7
0.010.81.21692.20u
HaWe 4
PN G149.4-09.2
1.000.81.241252.04nd
Sh 2-188
PN G128.0-04.1
1.810.831.311582.40nd
IsWe 2
PN G107.7+07.8
2.270.621.41261.89nd
Abell 74
PN G072.7-17.1
0.410.751.441081.62nd
Sh 2-176
PN G120.2-05.3
1.740.781.461041.73nd
Abell 29
PN G244.5+12.5
0.621.391.461021.69nd
WDHS 1
PN G197.4-06.4
0.310.852.391411.96o?
TK 1
PN G191.4+33.1
0.170.572.84991.80y?