2007ApJ...669..343C


Query : 2007ApJ...669..343C

2007ApJ...669..343C - Astrophys. J., 669, 343-362 (2007/November-1)

Spitzer IRAC observations of newly discovered planetary nebulae from the Macquarie-AAO-Strasbourg Hα planetary nebula project.

COHEN M., PARKER Q.A., GREEN A.J., MURPHY T., MISZALSKI B., FREW D.J., MEADE M.R., BABLER B., INDEBETOUW R., WHITNEY B.A., WATSON C., CHURCHWELL E.B. and WATSON D.F.

Abstract (from CDS):

We compare Hα, radio continuum, and Spitzer Space Telescope images of 58 planetary nebulae (PNe) recently discovered by the Macquarie-AAO-Strasbourg Hα PN Project (MASH) of the SuperCOSMOS Hα Survey. Using Infrared Array Camera (IRAC) data, we examine the relationships between optical and MIR morphologies from 3.6 to 8.0 µm and explore the ratio of mid-infrared (MIR) to radio nebular fluxes, which is a valuable discriminant between thermal and nonthermal emission. MASH emphasizes late evolutionary stages of PNe compared with previous catalogs, enabling study of the changes in MIR and radio flux that attend the aging process. Spatially integrated fluxes are constructed for all MASH PNe observed by the GLIMPSE Legacy Project, using the Hα morphologies to define the areas of MIR and radio continuum emission observed by the Midcourse Space Experiment (MSX), IRAC, the Molonglo Observatory Synthesis Telescope, and the Very Large Array (VLA). The ratio of IRAC 8.0 µm to MSX 8.3 µm fluxes provides an assessment of the absolute diffuse calibration of IRAC at 8.0 µm. We independently confirm the aperture correction factor to be applied to IRAC at 8.0 µm to align it with the diffuse calibration of MSX. The result is in accord with the recommendations of the Spitzer Science Center and with our results from a parallel study of H II regions in the MIR and radio. However, these PNe probe the diffuse calibration of IRAC on a spatial scale of 9"-77", as opposed to the many-arcminute scale from the H II regions' study.

Abstract Copyright: ∼

Journal keyword(s): Infrared: ISM - ISM: Planetary Nebulae: General - Radiation Mechanisms: Thermal - Radio Continuum: ISM - Space Vehicles

Simbad objects: 62

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Number of rows : 62
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 IC 418 PN 05 27 28.2059533560 -12 41 50.282287764   9.405 9.010 10.118   O7fp 1059 2
2 PN G295.9-00.4 PN? 11 50 07.0 -62 26 32           ~ 3 1
3 PN G296.2-00.4 PN? 11 52 55.7 -62 34 10           ~ 4 1
4 PN G296.8-00.9 PN? 11 57 03.2 -63 12 44           ~ 8 1
5 PN G297.5+01.0 PN 12 06 25.5 -61 22 44           ~ 4 1
6 PHR J1218-6245 PN? 12 18 00.9 -62 45 38           ~ 5 1
7 PN G299.7+00.1 PN 12 23 58.0 -62 36 21           ~ 7 1
8 NAME Coalsack Nebula DNe 12 31 19 -63 44.6           ~ 275 0
9 RCW 69 PN 12 44 27.4384824528 -62 31 18.880146408           ~ 24 1
10 WRAY 17-56 PN 12 46 26.9183160504 -63 24 27.881953452     16.9 15.1 15.553 ~ 21 1
11 PHR J1250-6346 PN 12 50 04.4 -63 46 52           ~ 8 1
12 PHR J1255-6251 PN 12 55 18.0 -62 51 04           ~ 7 1
13 PN G303.6+00.5 PN? 12 57 51.3 -62 16 12           ~ 7 1
14 WRAY 17-64 PN 14 08 47.10 -62 29 59.0     16.00     ~ 11 1
15 PHR J1408-6106 PN 14 08 51.7 -61 06 27           ~ 43 2
16 PN G314.9+00.5 PN? 14 29 43.9 -60 03 17           ~ 5 1
17 PN G314.6-00.1 PN? 14 29 53.0920465323 -60 43 56.219966359           ~ 10 1
18 PHR J1437-5949 PN 14 37 53.2 -59 49 25           ~ 9 1
19 PHR J1447-5838 PN 14 47 41.8 -58 38 41           ~ 6 1
20 PN G318.9+00.7 PN 14 57 35.7 -58 12 09           ~ 14 1
21 PN G319.5-01.0 PN 15 07 50.2 -59 25 14           ~ 6 1
22 PN G325.4-01.0 PN? 15 44 56.7 -56 07 07           ~ 3 1
23 PN G328.3+00.7 PN 15 52 56.8 -52 54 12           ~ 9 1
24 PN G331.2+00.0 PN? 16 10 21.1 -51 30 54           ~ 5 1
25 PMR 5 WR* 16 19 40.1905325832 -49 13 59.019951612           [WN6]: 37 2
26 PN G334.0+00.7 PN 16 19 50.1 -49 06 52           ~ 5 1
27 PN G332.3-00.9 PN? 16 19 57.5 -51 31 47           ~ 4 1
28 PN G333.2-00.6 PN? 16 22 40.6 -50 38 42           ~ 6 1
29 PN G337.3+00.6 PN 16 33 58.0 -46 50 07           ~ 13 1
30 PN G337.6+00.7 PN 16 34 51.2 -46 28 28           ~ 7 1
31 PHR J1635-4654 PN 16 35 51.9 -46 54 10           ~ 6 1
32 PHR J1639-4516 PN 16 39 22.3 -45 16 35           ~ 11 1
33 PN G339.9+00.5 PN? 16 44 36.2 -44 55 23           ~ 4 1
34 PN G340.8+00.8 PN? 16 46 27.6 -44 02 25           ~ 5 1
35 PN G347.0+00.3 PN 17 09 10.8 -39 31 06           ~ 10 1
36 NGC 6302 PN 17 13 44.5 -37 06 11           O-rich 821 2
37 PN G347.2-00.8 PN 17 14 49.1945959824 -40 06 07.367107860           ~ 11 1
38 PHR J1806-1956 PN 18 06 55.3 -19 56 18           ~ 11 1
39 PN G011.5+01.0 PN? 18 07 11.7 -18 27 54           ~ 6 1
40 PN G014.6+01.0 PN 18 13 28.9866765624 -15 43 19.848642096           ~ 9 1
41 PN G015.5+01.0 PN? 18 15 06.5 -14 57 21           ~ 9 1
42 PHR J1818-1526 PN 18 18 59.3239751160 -15 26 20.519836908           ~ 11 1
43 PN G017.2+00.1 PN? 18 21 43.9 -13 53 13           ~ 5 1
44 PN G016.4-00.9 PN 18 24 02.1 -15 05 33           ~ 7 1
45 PN G021.2+00.9 PN 18 26 26.1 -09 53 26           ~ 7 1
46 PN G023.4+00.7 PN 18 31 19.6 -08 05 43           ~ 8 1
47 PN G023.5-00.1 PN 18 34 41.6 -08 24 20           ~ 4 1
48 PN G027.5+01.0 PN? 18 38 02.25 -04 17 24.5           ~ 7 1
49 PN G026.8-00.5 PN? 18 42 17.9 -05 39 13           ~ 6 1
50 PN G029.5+00.6 PN? 18 42 57.1 -02 46 00           ~ 6 1
51 PN G026.9-00.7 PN 18 43 10.4 -05 41 51           ~ 6 1
52 PN G028.9+00.2 PN 18 43 15.3 -03 25 27           ~ 6 1
53 PHR J1843-0232 PN 18 43 56.9 -02 32 08           ~ 10 1
54 PN G027.7-00.6 PN 18 44 16.34 -04 52 52.0           ~ 5 1
55 PHR J1844-0503 PN 18 44 45.7 -05 03 54     13.2     ~ 14 2
56 PHR J1844-0517 PN 18 44 54.0 -05 17 36           ~ 6 1
57 PN G028.8-00.2 PN? 18 45 06.0 -03 43 33           ~ 8 1
58 PN G030.0+00.0 PN 18 46 02.7 -02 33 08           ~ 7 1
59 PHR J1847-0215 PN 18 47 47.4 -02 15 30           ~ 6 1
60 PN G033.9-00.9 PN 18 56 51.1 +00 28 53           ~ 5 1
61 PN G035.5-00.4 PN? 18 57 59.5 +02 07 07           ~ 20 1
62 NGC 7293 PN 22 29 38.5454047152 -20 50 13.747242408 11.894 13.158 13.524 13.689 13.898 DAO.5 983 1

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