Spitzer IRAC observations of newly-discovered planetary nebulae from the Macquarie-AAO-Strasbourg H-alpha Planetary Nebula Project
arXiv:0707.1347 · doi:10.1086/521427
Abstract
We compare H-alpha, radio continuum, and Spitzer Space Telescope (SST) images of 58 planetary nebulae (PNe) recently discovered by the Macquarie-AAO-Strasbo- urg H-alpha PN Project (MASH) of the SuperCOSMOS H-alpha Survey. Using InfraRed Array Camera (IRAC) data we define the IR colors of PNe and demonstrate good isolation between these colors and those of many other types of astronomical object. The only substantive contamination of PNe in the color-color plane we illustrate is due to YSOs. However, this ambiguity is readily resolved by the unique optical characteristics of PNe and their environs. We also examine the relationships between optical and MIR morphologies from 3.6 to 8.0um 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 MIR energy distributions were constructed for all MASH PNe observed by the GLIMPSE Legacy Project, using the H-alpha morphologies to establish the dimensions for the calculations of the Midcourse Space Experiment (MSX), IRAC, and radio continuum (from the Molonglo Observatory Synthesis Telescope and the Very Large Array) flux densities. The ratio of IRAC 8.0-um to MSX 8.3-um flux densities provides a measure of the absolute diffuse calibration of IRAC at 8.0 um. We independently confirm the aperture correction factor to be applied to IRAC at 8.0um to align it with the diffuse calibration of MSX. The result agrees with the recommendations of the Spitzer Science Center and with results from a parallel study of HII regions. These PNe probe the diffuse calibration of IRAC on a spatial scale of 9-77 arcsec.
48 pages, LaTeX (aastex), incl. 18 PostScript (eps) figures and 3 tables. Accepted by Astrophysical Journal
References in corpus (3)
Cited by in corpus (11)
- Intrinsically Red Sources observed by Spitzer in the Galactic Mid-Plane
- MASH-II: More Planetary Nebulae from the AAO/UKST HαSurvey
- New light on Galactic post-asymptotic giant branch stars. I. First distance catalogue
- Rings and Halos in the Mid-Infrared: The Planetary Nebulae NGC 7354 and NGC 3242
- The Halos of Planetary Nebulae in the Mid-Infrared: Evidence for Interaction with the Interstellar Medium
- MIPSGAL 24 μm Observations of Galactic Planetary Nebulae
- Mid and Far Infrared Photometry of Galactic Planetary Nebulae with the AKARI All Sky Survey
- Spitzer Mid-Infrared Observations of Seven Bipolar Planetary Nebulae
- Four New Planetary Nebulae Toward the Small Magellanic Cloud
- The nature of G52.381-0.849 and G56.240-0.345: young stellar objects associated with extended mid-infrared emission?
- Mid-Infrared Observations of Planetary Nebulae detected in the GLIMPSE 3D Survey