Planetary Nebula dust haloes revealed by Herschel
Paper in proceeding, 2013
Herschel Planetary Nebula Survey (HerPlaNS) is a far-IR imaging and spectroscopic survey of planetary nebulae, performedwith the Herschel Space Observatory, aiming at (1) establishing the spatially-resolved far-IR characteristics of the target nebulae and (2) understanding the energetics and shaping history of the circumstellar nebulae. Below we briefly demonstrate the breadth and depth of the HerPlaNS data set using one of the targets, NGC6781, as an example, and explore expectations in the era of SPICA, the next-generation far-IR mission.
Author
T. Ueta
University of Denver
Djazia Ladjal
University of Denver
K. M. Exter
KU Leuven
M. Otsuka
ASIAA Hilo Office
R. Szczerba
NCAC
N. Siódmiak
NCAC
I. Aleman
Leiden University
Aggm Tielens
KU Leuven
J. H. Kastner
RIT
J. Nordhaus
RIT
R. Montez
Vanderbilt University
I. McDonald
University of Manchester
K. Hebden
University of Manchester
A. Zijlstra
University of Manchester
M. Wittkowski
ESO
S. Ramstedt
Uppsala University
O. De Marco
Macquarie University
E. Villaver
UAM
B. Balick
University of Washington
E. Behar
Technion – Israel Institute of Technology
E. G. Blackman
University of Rochester
J. L. Hora
CfA/Harvard
Y. H. Chu
UIUC
H. Izumiura
OAO/NAOJ
J. A. Lopez
Universidad Nacional Autónoma de México
K. Murakawa
University of Leeds
R. Nordon
MPE
C. Sandin
AIP
R. Sahai
JPL
P. A. M. van Hoof
Royal Observatory of Belgium
Wouter Vlemmings
Chalmers, Earth and Space Sciences, Radio Astronomy and Astrophysics
I. Yamamura
JAXA Institute of Space and Astronautical Science
Proceedings of Science
18248039 (eISSN)
The Life Cycle of Dust in the Universe: Observations, Theory, and Laboratory Experiments
Tapei, Taiwan,
Tapei, Taiwan,
Subject Categories
Astronomy, Astrophysics and Cosmology
DOI
10.22323/1.207.0050