The dust morphology of the elliptical Galaxy M 86 with SPIRE

H.L. Gomez; M. Baes; Luca Cortese; M.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; J.A. 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
, Luca Cortese
, M.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, J.A. Stevens, M. Symeonidis, M. Trichas, M. Vaccari, L. Vigroux, C.D. Wilson, H. Wozniak, G.S. Wright, W.W. Zeilinger

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46 Citations (Scopus)

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 Modot; 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. © ESO 2010.

Original language	English
Pages (from-to)	5
Journal	Astronomy and Astrophysics
Volume	518
Issue number	4
DOIs	https://doi.org/10.1051/0004-6361/201014530
Publication status	Published - 2010

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Gomez, H. L., Baes, M., Cortese, L., Smith, M. 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 and Astrophysics, 518(4), 5. https://doi.org/10.1051/0004-6361/201014530

@article{4dc610095b904585bd076f9306501859,

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 ∼106 Modot; 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. {\textcopyright} ESO 2010.",

author = "H.L. Gomez and M. Baes and Luca Cortese and M.L. Smith and A. Boselli and L. Ciesla and G.J. Bendo and M. Pohlen and \{Di Serego Alighieri\}, S. and R. Auld and M.J. Barlow and J.J. Bock and M. Bradford and V. Buat and N. Castro-Rodriguez and P. Chanial and S. Charlot and D.L. Clements and A. Cooray and D. Cormier and J.I. Davies 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 L.R. Levenson 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 E.E. Rigby and H. Roussel and A. Rykala and N. Sacchi and M. Sauvage and M.R.P. Schirm and B. Schulz and L. Spinoglio and S. Srinivasan and J.A. 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",

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

language = "English",

volume = "518",

pages = "5",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "4",

}

Gomez, HL, Baes, M, Cortese, L, Smith, ML, 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, JA, 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 and Astrophysics, vol. 518, no. 4, pp. 5. 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, Luca

AU - Smith, M.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, J.A.

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

Y1 - 2010

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 Modot; 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. © ESO 2010.

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 Modot; 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. © ESO 2010.

U2 - 10.1051/0004-6361/201014530

DO - 10.1051/0004-6361/201014530

M3 - Article

SN - 0004-6361

VL - 518

SP - 5

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 4

ER -

The dust morphology of the elliptical Galaxy M 86 with SPIRE

Abstract

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