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The dust morphology of the elliptical Galaxy M 86 with SPIRE

HL Gomez, Maarten Baes UGent, L Cortese, MWL Smith, A Boselli, L Ciesla, GJ Bendo, M Pohlen, SD Alighieri and R Auld, et al. (2010) ASTRONOMY & ASTROPHYSICS. 518.
abstract
We present Herschel-SPIRE observations at 250-500 mu m of the giant elliptical galaxy M 86 and examine the distribution of the resolved cold dust emission and its relation with other galactic tracers. The SPIRE images reveal three dust components: emission from the central region; a dust lane extending north-south; and a bright emission feature 10 kpc to the south-east. We estimate that similar to 10(6) M-circle dot of dust is spatially coincident with atomic and ionized hydrogen, originating from stripped material from the nearby spiral NGC 4438 due to recent tidal interactions with M 86. The gas-to-dust ratio of the cold gas component ranges from similar to 20-80. We discuss the different heating mechanisms for the dust features.
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle (original)
publication status
published
subject
keyword
cD, galaxies: individual: M 86, galaxies: ellipticals and lenticular, submillimeter: ISM, dust, extinction, MULTIPHASE INTERSTELLAR-MEDIUM, VIRGO CLUSTER, COLD DUST, GAS, EMISSION, NGC-4406, M-86, M86
journal title
ASTRONOMY & ASTROPHYSICS
Astron. Astrophys.
volume
518
issue title
Herschel: the first science highlights
article_number
L45
pages
5 pages
Web of Science type
Article
Web of Science id
000281527200046
JCR category
ASTRONOMY & ASTROPHYSICS
JCR impact factor
4.41 (2010)
JCR rank
10/54 (2010)
JCR quartile
1 (2010)
ISSN
0004-6361
DOI
10.1051/0004-6361/201014530
language
English
UGent publication?
yes
classification
A1
copyright statement
I have transferred the copyright for this publication to the publisher
id
1236520
handle
http://hdl.handle.net/1854/LU-1236520
date created
2011-05-25 11:24:22
date last changed
2011-06-06 15:18:59
@article{1236520,
  abstract     = {We present Herschel-SPIRE observations at 250-500 mu m of the giant elliptical galaxy M 86 and examine the distribution of the resolved cold dust emission and its relation with other galactic tracers. The SPIRE images reveal three dust components: emission from the central region; a dust lane extending north-south; and a bright emission feature 10 kpc to the south-east. We estimate that similar to 10(6) M-circle dot of dust is spatially coincident with atomic and ionized hydrogen, originating from stripped material from the nearby spiral NGC 4438 due to recent tidal interactions with M 86. The gas-to-dust ratio of the cold gas component ranges from similar to 20-80. We discuss the different heating mechanisms for the dust features.},
  articleno    = {L45},
  author       = {Gomez, HL and Baes, Maarten and Cortese, L and Smith, MWL and Boselli, A and Ciesla, L and Bendo, GJ and Pohlen, M and Alighieri, SD and Auld, R and Barlow, MJ and Bock, JJ and Bradford, M and Buat, V and Castro-Rodriguez, N and Chanial, P and Charlot, S and Clements, DL and Cooray, A and Cormier, D and Davies, JI and Dwek, E and Eales, S and Elbaz, D and Galametz, M and Galliano, F and Gear, WK and Glenn, J and Griffin, M and Hony, S and Isaak, KG and Levenson, LR and Lu, N and Madden, S and O'Halloran, B and Okumura, K and Oliver, S and Page, MJ and Panuzzo, P and Papageorgiou, A and Parkin, TJ and Perez-Fournon, I and Rangwala, N and Rigby, EE and Roussel, H and Rykala, A and Sacchi, N and Sauvage, M and Schirm, MRP and Schulz, B and Spinoglio, L and Srinivasan, S and Stevens, JA and Symeonidis, M and Trichas, M and Vaccari, M and Vigroux, L and Wilson, CD and Wozniak, H and Wright, GS and Zeilinger, WW},
  issn         = {0004-6361},
  journal      = {ASTRONOMY \& ASTROPHYSICS},
  keyword      = {cD,galaxies: individual: M 86,galaxies: ellipticals and lenticular,submillimeter: ISM,dust,extinction,MULTIPHASE INTERSTELLAR-MEDIUM,VIRGO CLUSTER,COLD DUST,GAS,EMISSION,NGC-4406,M-86,M86},
  language     = {eng},
  pages        = {5},
  title        = {The dust morphology of the elliptical Galaxy M 86 with SPIRE},
  url          = {http://dx.doi.org/10.1051/0004-6361/201014530},
  volume       = {518},
  year         = {2010},
}

Chicago
Gomez, HL, Maarten Baes, L Cortese, MWL Smith, A Boselli, L Ciesla, GJ Bendo, et al. 2010. “The Dust Morphology of the Elliptical Galaxy M 86 with SPIRE.” Astronomy & Astrophysics 518.
APA
Gomez, H., Baes, M., Cortese, L., Smith, M., Boselli, A., Ciesla, L., Bendo, G., et al. (2010). The dust morphology of the elliptical Galaxy M 86 with SPIRE. ASTRONOMY & ASTROPHYSICS, 518.
Vancouver
1.
Gomez H, Baes M, Cortese L, Smith M, Boselli A, Ciesla L, et al. The dust morphology of the elliptical Galaxy M 86 with SPIRE. ASTRONOMY & ASTROPHYSICS. 2010;518.
MLA
Gomez, HL, Maarten Baes, L Cortese, et al. “The Dust Morphology of the Elliptical Galaxy M 86 with SPIRE.” ASTRONOMY & ASTROPHYSICS 518 (2010): n. pag. Print.