CaltechAUTHORS
  A Caltech Library Service

The Nature of Dust in Compact Galactic Planetary Nebulae from Spitzer Spectra

Stanghellini, Letizia and García-Hernández, D. A. and García-Lario, Pedro and Davies, James E. and Shaw, Richard A. and Villaver, Eva and Manchado, Arturo and Perea-Calderón, Jose V. (2012) The Nature of Dust in Compact Galactic Planetary Nebulae from Spitzer Spectra. Astrophysical Journal, 753 (2). Art. No. 172 . ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20120730-114046528

[img]
Preview
PDF - Published Version
See Usage Policy.

1118Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20120730-114046528

Abstract

We present the Spitzer/Infrared Spectrograph (IRS) spectra of 157 compact Galactic planetary nebulae (PNe). These young PNe provide insight on the effects of dust in early post-asymptotic giant branch evolution, before much of the dust is altered or destroyed by the hardening stellar radiation field. Most of the selected targets have PN-type IRS spectra, while a few turned out to be misclassified stars. We inspected the group properties of the PN spectra and classified them based on the different dust classes (featureless or F, carbon-rich dust or CRD, oxygen-rich dust or ORD, mixed-chemistry dust or MCD) and subclasses (aromatic and aliphatic, and crystalline and amorphous). All PNe are characterized by dust continuum and more than 80% of the sample shows solid-state features above the continuum, in contrast with the Magellanic Cloud sample where only ~40% of the entire sample displays solid-state features; this is an indication of the strong link between dust properties and metallicity. The Galactic PNe that show solid-state features are almost equally divided among the CRD, ORD, and MCD. We analyzed dust properties together with other PN properties and found that (1) there is an enhancement of MCD PNe toward the Galactic center, in agreement with studies of Galactic bulge PNe; (2) CRD PNe could be seen as defining an evolutionary sequence, contrary to the ORD and MCD PNe, which are scattered in all evolutionary diagrams; (3) carbon-rich and oxygen-rich grains retain different equilibrium temperatures, as expected from models; and (4) ORD PNe are highly asymmetric, i.e., bipolar or bipolar core, and CRD PNe highly symmetric, i.e., round or elliptical; point symmetry is statistically more common in MCD than in other dust class PNe. By comparing the sample of this paper to that of Magellanic Cloud PNe, we find that the latter sample does not include MCD PNe, and the other dust classes are differently populated, with continuity of the fraction of F, CRD, ORD, and MCD populations from high to low metallicity environments. We also find similar sequences for CRD PNe in the Galactic disk and the Magellanic Clouds, except that the Magellanic Cloud PNe seem to attain higher dust temperatures at similar evolutionary stages, in agreement with the observational findings of smaller dust grains (i.e., lower radiation efficiency) in low metallicity interstellar environments.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/0004-637X/753/2/172DOIUNSPECIFIED
http://iopscience.iop.org/0004-637X/753/2/172PublisherUNSPECIFIED
Additional Information:© 2012 American Astronomical Society. Received 2011 August 10; accepted 2012 May 8; published 2012 June 26. Support for this work was provided by NASA through a grant issued by JPL/Caltech for Spitzer Program GO 50261. We acknowledge support from the Faculty of the European Space Astronomy Centre (ESAC). D.A.G.H. and A.M. also acknowledge support provided by the Spanish Ministry of Science and Innovation (MICINN) under a 2008 JdC grant and under grant AYA-2007-64748. We thank an anonymous referee for helping us improve a previous version of this paper. E.V. acknowledges support provided by the Spanish Ministry of Science and Innovation (MICINN) under grant AYA2010-20630 and to the Marie Curie FP7-People-RG268111. Based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA.
Funders:
Funding AgencyGrant Number
NASA Spitzer Program GO 50261
Faculty of the European Space Astronomy Centre (ESAC)UNSPECIFIED
Spanish Ministry of Science and Innovation (MICINN)2008 JdC
Spanish Ministry of Science and Innovation (MICINN)AYA-2007-64748
Spanish Ministry of Science and Innovation (MICINN)AYA2010-20630
Marie Curie FP7RG268111
Subject Keywords:planetary nebulae: general
Issue or Number:2
Record Number:CaltechAUTHORS:20120730-114046528
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20120730-114046528
Official Citation:The Nature of Dust in Compact Galactic Planetary Nebulae from Spitzer Spectra Letizia Stanghellini et al. 2012 ApJ 753 172
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:32791
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:30 Jul 2012 20:09
Last Modified:03 Oct 2019 04:04

Repository Staff Only: item control page