The Herschel Virgo Cluster Survey. III. A constraint on dust grain lifetime in early-type galaxies

@article{Clemens2010TheHV,
  title={The Herschel Virgo Cluster Survey. III. A constraint on dust grain lifetime in early-type galaxies},
  author={Marcel Clemens and A. P. Jones and Alessandro Bressan and Maarten Baes and George J Bendo and Stefano Bianchi and Dominik J. Bomans and Alessandro Boselli and Edvige Corbelli and Luca Cortese and Ali A. Dariush and Jonathan Ivor Davies and I. De Looze and Sperello di Serego Alighieri and Dario Fadda and Jacopo Fritz and Diego Garcia-Appadoo and Giuseppe Gavazzi and Carlo Giovanardi and Marco Grossi and Thomas M. Hughes and Leslie K. Hunt and S. Madden and Daniele Pierini and Michael Pohlen and Silvio P. Sabatini and M. W. L. Smith and J. Verstappen and Catherine Vlahakis and Emmanuel M. Xilouris and Stefano Zibetti},
  journal={Astronomy and Astrophysics},
  year={2010},
  volume={518},
  pages={1-4}
}
Passive early-type galaxies (ETGs) provide an ideal laboratory for studying the interplay between dust formation around evolved stars and its subsequent destruction in a hot gas. Using Spitzer-IRS and Herschel data we compare the dust production rate in the envelopes of evolved AGB stars with a constraint on the total dust mass. Early-type galaxies which appear to be truly passively evolving are not detected by Herschel. We thus derive a distance independent upper limit to the dust grain… 

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References

SHOWING 1-10 OF 36 REFERENCES

Interstellar Grains in Elliptical Galaxies: Grain Evolution

We consider the lifecycle of dust introduced into the hot interstellar medium in isolated elliptical galaxies. Dust grains are ejected into galactic-scale cooling flows in large ellipticals by normal

The Herschel Virgo Cluster Survey - II. Truncated dust disks in H I-deficient spirals

By combining Herschel-SPIRE observations obtained as part of the Herschel Virgo Cluster Survey with 21 cm Hi data from the literature, we investigate the role of the cluster environment on the dust

The Star Formation History of the Virgo Early-Type Galaxy NGC 4435: The Spitzer Mid-Infrared View

We present a population synthesis study of NGC 4435, an early-type Virgo galaxy interacting with NGC 4438. We combine new spectroscopic observations obtained with the Spitzer Space Telescope IRS

Far-Infrared Spitzer Observations of Elliptical Galaxies: Evidence for Extended Diffuse Dust

Far-infrared Spitzer observations of elliptical galaxies are inconsistent with simple steady state models of dust creation in red giant stars and destruction by grain sputtering in the hot

Spitzer IRS spectra of Virgo Early-Type Galaxies: Detection of Stellar Silicate Emission

We present high signal-to-noise ratio Spitzer Infrared Spectrograph observations of 17 Virgo early-type galaxies. The galaxies were selected from those that define the color-magnitude relation of the

Dust in Hot Plasma of Nearby Dusty Elliptical Galaxies Observed with the Spitzer Space Telescope

We report on mid- and far-IR Spitzer observations of 7 nearby dusty elliptical galaxies by using the Multiband Imaging Photometer (MIPS) and Infrared Spectrograph (IRS). Our sample galaxies are known

Accretion and Nuclear Activity of Quiescent Supermassive Black Holes. I. X-Ray Study

We have studied the nuclear activity in a sample of six quiescent early-type galaxies, with new Chandra data and archival HST optical images. Their nuclear sources have X-ray luminosities ~1038-1039

The Herschel Virgo Cluster Survey. I. Luminosity function [Letter]

We describe the Herschel Virgo Cluster Survey (HeViCS) and the first data obtained as part of the science demonstration phase (SDP). The data cover a central 4×4 sq deg region of the cluster. We use

Nuclear Accretion in Galaxies of the Local Universe: Clues from Chandra Observations

In order to find an explanation for the radiative quiescence of supermassive black holes in the local universe, the most accurate estimates for a sample of nearby galaxies are collected for the mass

Interaction between the intergalactic medium and galactic outflows from dwarf galaxies

We have carried out two-dimensional (2D) hydrodynamical simulations in order to study the interaction between supernova-powered gas outflows from low-mass galaxies and the local intergalactic medium