The Herschel Virgo Cluster Survey: VII. Dust in cluster dwarf elliptical galaxies
arXiv:1005.3060 · doi:10.1051/0004-6361/201014647
Abstract
We use the Science Demonstration Phase data of the Herschel Virgo Cluster Survey to search for dust emission of early-type dwarf galaxies in the central regions of the Virgo Cluster as an alternative way of identifying the interstellar medium.We present the first possible far-infrared detection of cluster early-type dwarf galaxies: VCC781 and VCC951 are detected at the 10 sigma level in the SPIRE 250 micron image. Both detected galaxies have dust masses of the order of 10^5 Msun and average dust temperatures ~20K. The detection rate (less than 1%) is quite high compared to the 1.7% detection rate for Hi emission, considering that dwarfs in the central regions are more Hi deficient. We conclude that the removal of interstellar dust from dwarf galaxies resulting from ram pressure stripping, harassment, or tidal effects must be as efficient as the removal of interstellar gas.
Letter accepted for publication in A&A (Herschel special issue)
References in corpus (16)
- Herschel Space Observatory - An ESA facility for far-infrared and submillimetre astronomy
- The Photodetector Array Camera and Spectrometer (PACS) on the Herschel Space Observatory
- The Herschel-SPIRE instrument and its in-flight performance
- The origin of dwarf ellipticals in the Virgo cluster
- Virgo cluster early-type dwarf galaxies with the Sloan Digital Sky Survey. I. On the possible disk nature of bright early-type dwarfs
- The Arecibo Legacy Fast ALFA Survey: III. HI Source Catalog of the Northern Virgo Cluster Region
- Virgo cluster early-type dwarf galaxies with the Sloan Digital Sky Survey. II. Early-type dwarfs with central star formation
- The Herschel Virgo Cluster Survey: II. Truncated dust disks in HI-deficient spirals
- The Herschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754
- The Herschel Virgo Cluster Survey: I. Luminosity functions
- Simulations of the formation and evolution of isolated dwarf galaxies
- The origin of the mu_e - M_B and Kormendy relations in dwarf elliptical galaxies
- The HI content of Early-Type Galaxies from the ALFALFA survey I. Catalogued HI sources in the Virgo cluster
- Kinematic properties as probes of the evolution of dwarf galaxies in the Virgo cluster
- Spitzer Observations of Low Luminosity Isolated and Low Surface Brightness Galaxies
- Mapping and Mass Measurement of the Cold Dust in NGC 205 with Spitzer
Cited by in corpus (39)
- Three-dimensional radiative transfer modeling of AGN dusty tori as a clumpy two-phase medium
- Efficient 3D NLTE dust radiative transfer with SKIRT
- Ram Pressure Stripping in High-Density Environments
- The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
- On the origin of the faint-end of the red sequence in high density environments
- The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV: The role of the cluster environment on galaxy evolution
- MIPS 24-160 micron photometry for the Herschel-SPIRE Local Galaxies Guaranteed Time Programs
- The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). I: The UV luminosity function of the central 12 sq.deg
- The ALMA Fornax Cluster Survey I: stirring and stripping of the molecular gas in cluster galaxies
- The Star Formation Rate-Density Relation at 0.6<z<0.9 and the Role of Star Forming Galaxies
- The Herschel Virgo Cluster Survey XII: FIR properties of optically-selected Virgo Cluster galaxies
- The Herschel Virgo Cluster Survey: I. Luminosity functions
- A near-infrared census of the multi-component stellar structure of early-type dwarf galaxies in the Virgo cluster
- The dust energy balance in the edge-on spiral galaxy NGC 4565
- The Herschel Virgo Cluster Survey - VIII. The Bright Galaxy Sample
- Dissecting early-type dwarf galaxies into their multiple components
- FitSKIRT: genetic algorithms to automatically fit dusty galaxies with a Monte Carlo radiative transfer code
- Virgo Redux: The Masses and Stellar Content of Nuclei in Early-Type Galaxies from Multi-Band Photometry and Spectroscopy
- Panchromatic radiative transfer modeling of stars and dust in the Sombrero galaxy
- Dwarf galaxy populations in present-day galaxy clusters - II. The history of early-type and late-type dwarfs
- The Next Generation Virgo Cluster Survey. VII. The intrinsic shapes of low-luminosity galaxies in the core of the Virgo cluster, and a comparison with the Local Group
- Simulations of the formation and evolution of isolated dwarf galaxies - II. Angular momentum as a second parameter
- The properties of early-type galaxies in the Ursa Major cluster
- The Herschel Fornax Cluster Survey I: The Bright Galaxy Sample
- Young stellar populations in early-type dwarf galaxies; occurrence, radial extent and scaling relations
- Young, metal-enriched cores in early-type dwarf galaxies in the Virgo cluster based on colour gradients
- The Herschel Virgo Cluster Survey XVI: a cluster inventory
- High-resolution, 3D radiative transfer modelling IV. AGN-powered dust heating in NGC 1068
- The Occulting Galaxy Pair UGC 3995; Dust properties from HST and CALIFA data
- H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
- The Herschel Virgo Cluster Survey XIV: transition-type dwarf galaxies in the Virgo cluster
- Dark Matter and IMF normalization in Virgo dwarf early-type galaxies
- Gravitational microlensing of AGN dusty tori
- The interstellar medium in Andromeda's dwarf spheroidal galaxies: I. Content and origin of the interstellar dust
- The Herschel Fornax Cluster Survey II: FIR properties of optically-selected Fornax cluster galaxies
- Formation of Blue-cored Dwarf Early-type Galaxies in a Cluster Environment: a Kinematical Perspective
- The Herschel Virgo Cluster Survey. XV. Planck submillimetre sources in the Virgo Cluster
- Radiative transfer in disc galaxies V. The accuracy of the KB approximation
- The influence of the Cosmic Web on the properties of dwarf galaxies in the Fornax-Eridanus Supercluster