The dust morphology of the elliptical Galaxy M 86 with SPIRE

H.L. Gomez; M. Baes; L. Cortese; M. W. L. Smith; A. Boselli; L. Ciesla; G. J. Bendo; M. Pohlen; S. di Serego Alighieri; R. Auld; M.J. Barlow; J. J. Bock; M. Bradford; V. Buat; N. Castro-Rodriguez; P. Chanial; S. Charlot; D. L. Clements; A. Cooray; D. Cormier; J. I. Davies; E. Dwek; S. Eales; D. Elbaz; M. Galametz; F. Galliano; W.K. Gear; J. Glenn; M. Griffin; S. Hony; K.G. Isaak; L. R. Levenson; N. Lu; S. Madden; B. O'Halloran; K. Okumura; S. Oliver; M.J. Page; P. Panuzzo; A. Papageorgiou; T.J. Parkin; I. Perez-Fournon; N. Rangwala; E. E. Rigby; H. Roussel; A. Rykala; N. Sacchi; M. Sauvage; M. R. P. Schirm; B. Schulz; L. Spinoglio; S. Srinivasan; Jason Stevens; M. Symeonidis; M. Trichas; M. Vaccari; L. Vigroux; C.D. Wilson; H. Wozniak; G.S. Wright; W.W. Zeilinger

doi:10.1051/0004-6361/201014530

The dust morphology of the elliptical Galaxy M 86 with SPIRE

H.L. Gomez
, M. Baes
, L. Cortese
, M. W. L. Smith
, A. Boselli
, L. Ciesla
, G. J. Bendo
, M. Pohlen
, S. di Serego Alighieri
, R. Auld
, M.J. Barlow
, J. J. Bock
, M. Bradford
, V. Buat
, N. Castro-Rodriguez
, P. Chanial
, S. Charlot
, D. L. Clements
, A. Cooray
, D. Cormier

J. I. Davies, E. Dwek, S. Eales, D. Elbaz, M. Galametz, F. Galliano, W.K. Gear, J. Glenn, M. Griffin, S. Hony, K.G. Isaak, L. R. Levenson, N. Lu, S. Madden, B. O'Halloran, K. Okumura, S. Oliver, M.J. Page, P. Panuzzo, A. Papageorgiou, T.J. Parkin, I. Perez-Fournon, N. Rangwala, E. E. Rigby, H. Roussel, A. Rykala, N. Sacchi, M. Sauvage, M. R. P. Schirm, B. Schulz, L. Spinoglio, S. Srinivasan, Jason Stevens, M. Symeonidis, M. Trichas, M. Vaccari, L. Vigroux, C.D. Wilson, H. Wozniak, G.S. Wright, W.W. Zeilinger

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Abstract

We present Herschel-SPIRE observations at 250–500 μm 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 ~10⁶ M ? 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 ~20–80. We discuss the different heating mechanisms for the dust features.

Original language	English
Article number	L45
Journal	Astronomy & Astrophysics
Volume	518
DOIs	https://doi.org/10.1051/0004-6361/201014530
Publication status	Published - 1 Jul 2010

Keywords

galaxies: ellipticals and lenticular, cD, galaxies: individual: M 86, submillimeter: ISM, dust, extinction

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10.1051/0004-6361/201014530

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Gomez, H. L., Baes, M., Cortese, L., Smith, M. W. L., Boselli, A., Ciesla, L., Bendo, G. J., Pohlen, M., di Serego Alighieri, S., Auld, R., Barlow, M. J., Bock, J. J., Bradford, M., Buat, V., Castro-Rodriguez, N., Chanial, P., Charlot, S., Clements, D. L., Cooray, A., ... Zeilinger, W. W. (2010). The dust morphology of the elliptical Galaxy M 86 with SPIRE. Astronomy & Astrophysics, 518, Article L45. https://doi.org/10.1051/0004-6361/201014530

@article{d447e16c6b5c470bb075639e9ffbb4ea,

title = "The dust morphology of the elliptical Galaxy M 86 with SPIRE",

abstract = "We present Herschel-SPIRE observations at 250–500 μm 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 \textasciitilde{}106 M ? 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 \textasciitilde{}20–80. We discuss the different heating mechanisms for the dust features.",

keywords = "galaxies: ellipticals and lenticular, cD, galaxies: individual: M 86, submillimeter: ISM, dust, extinction",

author = "H.L. Gomez and M. Baes and L. Cortese and Smith, \{M. W. L.\} and A. Boselli and L. Ciesla and Bendo, \{G. J.\} and M. Pohlen and \{di Serego Alighieri\}, S. and R. Auld and M.J. Barlow and Bock, \{J. J.\} and M. Bradford and V. Buat and N. Castro-Rodriguez and P. Chanial and S. Charlot and Clements, \{D. L.\} and A. Cooray and D. Cormier and Davies, \{J. I.\} and E. Dwek and S. Eales and D. Elbaz and M. Galametz and F. Galliano and W.K. Gear and J. Glenn and M. Griffin and S. Hony and K.G. Isaak and Levenson, \{L. R.\} and N. Lu and S. Madden and B. O'Halloran and K. Okumura and S. Oliver and M.J. Page and P. Panuzzo and A. Papageorgiou and T.J. Parkin and I. Perez-Fournon and N. Rangwala and Rigby, \{E. E.\} and H. Roussel and A. Rykala and N. Sacchi and M. Sauvage and Schirm, \{M. R. P.\} and B. Schulz and L. Spinoglio and S. Srinivasan and Jason Stevens and M. Symeonidis and M. Trichas and M. Vaccari and L. Vigroux and C.D. Wilson and H. Wozniak and G.S. Wright and W.W. Zeilinger",

year = "2010",

month = jul,

day = "1",

doi = "10.1051/0004-6361/201014530",

language = "English",

volume = "518",

journal = "Astronomy \& Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Gomez, HL, Baes, M, Cortese, L, Smith, MWL, Boselli, A, Ciesla, L, Bendo, GJ, Pohlen, M, di Serego Alighieri, S, Auld, R, Barlow, MJ, Bock, JJ, Bradford, M, Buat, V, Castro-Rodriguez, N, Chanial, P, Charlot, S, Clements, DL, Cooray, A, Cormier, D, Davies, JI, Dwek, E, Eales, S, Elbaz, D, Galametz, M, Galliano, F, Gear, WK, Glenn, J, Griffin, M, Hony, S, Isaak, KG, Levenson, LR, Lu, N, Madden, S, O'Halloran, B, Okumura, K, Oliver, S, Page, MJ, Panuzzo, P, Papageorgiou, A, Parkin, TJ, Perez-Fournon, I, Rangwala, N, Rigby, EE, Roussel, H, Rykala, A, Sacchi, N, Sauvage, M, Schirm, MRP, Schulz, B, Spinoglio, L, Srinivasan, S, Stevens, J, Symeonidis, M, Trichas, M, Vaccari, M, Vigroux, L, Wilson, CD, Wozniak, H, Wright, GS & Zeilinger, WW 2010, 'The dust morphology of the elliptical Galaxy M 86 with SPIRE', Astronomy & Astrophysics, vol. 518, L45. https://doi.org/10.1051/0004-6361/201014530

TY - JOUR

T1 - The dust morphology of the elliptical Galaxy M 86 with SPIRE

AU - Gomez, H.L.

AU - Baes, M.

AU - Cortese, L.

AU - Smith, M. W. L.

AU - Boselli, A.

AU - Ciesla, L.

AU - Bendo, G. J.

AU - Pohlen, M.

AU - di Serego Alighieri, S.

AU - Auld, R.

AU - Barlow, M.J.

AU - Bock, J. J.

AU - Bradford, M.

AU - Buat, V.

AU - Castro-Rodriguez, N.

AU - Chanial, P.

AU - Charlot, S.

AU - Clements, D. L.

AU - Cooray, A.

AU - Cormier, D.

AU - Davies, J. I.

AU - Dwek, E.

AU - Eales, S.

AU - Elbaz, D.

AU - Galametz, M.

AU - Galliano, F.

AU - Gear, W.K.

AU - Glenn, J.

AU - Griffin, M.

AU - Hony, S.

AU - Isaak, K.G.

AU - Levenson, L. R.

AU - Lu, N.

AU - Madden, S.

AU - O'Halloran, B.

AU - Okumura, K.

AU - Oliver, S.

AU - Page, M.J.

AU - Panuzzo, P.

AU - Papageorgiou, A.

AU - Parkin, T.J.

AU - Perez-Fournon, I.

AU - Rangwala, N.

AU - Rigby, E. E.

AU - Roussel, H.

AU - Rykala, A.

AU - Sacchi, N.

AU - Sauvage, M.

AU - Schirm, M. R. P.

AU - Schulz, B.

AU - Spinoglio, L.

AU - Srinivasan, S.

AU - Stevens, Jason

AU - Symeonidis, M.

AU - Trichas, M.

AU - Vaccari, M.

AU - Vigroux, L.

AU - Wilson, C.D.

AU - Wozniak, H.

AU - Wright, G.S.

AU - Zeilinger, W.W.

PY - 2010/7/1

Y1 - 2010/7/1

N2 - We present Herschel-SPIRE observations at 250–500 μm 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 ~106 M ? 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 ~20–80. We discuss the different heating mechanisms for the dust features.

AB - We present Herschel-SPIRE observations at 250–500 μm 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 ~106 M ? 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 ~20–80. We discuss the different heating mechanisms for the dust features.

KW - galaxies: ellipticals and lenticular, cD, galaxies: individual: M 86, submillimeter: ISM, dust, extinction

U2 - 10.1051/0004-6361/201014530

DO - 10.1051/0004-6361/201014530

M3 - Article

SN - 0004-6361

VL - 518

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - L45

ER -

The dust morphology of the elliptical Galaxy M 86 with SPIRE

Abstract

Keywords

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