Mapping the interstellar medium in galaxies with Herschel*/SPIRE

S. A. Eales; M. W.L. Smith; C. D. Wilson; G. J. Bendo; L. Cortese; M. Pohlen; A. Boselli; H. L. Gomez; R. Auld; M. Baes; M. J. Barlow; J. J. Bock; M. Bradford; V. Buat; N. Castro-Rodríguez; P. Chanial; S. Charlot; L. Ciesla; D. L. Clements; A. Cooray; D. Cormier; J. I. Davies; E. Dwek; D. Elbaz; M. Galametz; F. Galliano; W. K. Gear; J. Glenn; M. Griffin; S. Hony; K. 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. Pérez-Fournon; N. Rangwala; E. E. Rigby; H. Rousse; A. Rykala; N. Sacchi; M. Sauvage; B. Schulz; M. R.P. Schirm; L. Spinoglio; S. Srinivasan; J. A. Stevens; M. Symeonidis; M. Trichas; M. Vaccari; L. Vigroux; H. Wozniak; G. S. Wright; W. W. Zeilinger

doi:10.1051/0004-6361/201014536

Mapping the interstellar medium in galaxies with Herschel*/SPIRE

S. A. Eales
, M. W.L. Smith
, C. D. Wilson
, G. J. Bendo
, L. Cortese
, M. Pohlen
, A. Boselli
, H. L. Gomez
, R. Auld
, M. Baes
, M. J. Barlow
, J. J. Bock
, M. Bradford
, V. Buat
, N. Castro-Rodríguez
, P. Chanial
, S. Charlot
, L. Ciesla
, D. L. Clements
, A. Cooray

D. Cormier, J. I. Davies, E. Dwek, D. Elbaz, M. Galametz, F. Galliano, W. K. Gear, J. Glenn, M. Griffin, S. Hony, K. 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. Pérez-Fournon, N. Rangwala, E. E. Rigby, H. Rousse, A. Rykala, N. Sacchi, M. Sauvage, B. Schulz, M. R.P. Schirm, L. Spinoglio, S. Srinivasan, J. A. Stevens, M. Symeonidis, M. Trichas, M. Vaccari, L. Vigroux, H. Wozniak, G. S. Wright, W. W. Zeilinger

Research output: Contribution to a Journal (Peer & Non Peer) › Article › peer-review

36 Citations (Scopus)

Abstract

The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter, we use SPIRE observations of the galaxies M 99 and M 100 to explore the alternative approach of mapping the interstellar medium using the continuum emission from the dust. We have compared the methods by measuring the relationship between the star-formation rate and the surface density of gas in the galaxies using both methods. We find the two methods give relationships with a similar dispersion, confirming that observing the continuum emission from the dust is a promising method of mapping the interstellar medium in galaxies.

Original language	English
Article number	L62
Journal	Astronomy and Astrophysics
Volume	518
Issue number	4
DOIs	https://doi.org/10.1051/0004-6361/201014536
Publication status	Published - 2010
Externally published	Yes

UN SDGs

This output contributes to the following UN Sustainable Development Goals (SDGs)

SDG 13 Climate Action

Keywords

ISM: abundances
dust, extinction
galaxies: ISM
galaxies: spiral

Access to Document

10.1051/0004-6361/201014536

Cite this

Eales, S. A., Smith, M. W. L., Wilson, C. D., Bendo, G. J., Cortese, L., Pohlen, M., Boselli, A., Gomez, H. L., Auld, R., Baes, M., Barlow, M. J., Bock, J. J., Bradford, M., Buat, V., Castro-Rodríguez, N., Chanial, P., Charlot, S., Ciesla, L., Clements, D. L., ... Zeilinger, W. W. (2010). Mapping the interstellar medium in galaxies with Herschel*/SPIRE. Astronomy and Astrophysics, 518(4), Article L62. https://doi.org/10.1051/0004-6361/201014536

@article{27172d4c2d72498d98fddb169dcb8c9f,

title = "Mapping the interstellar medium in galaxies with Herschel*/SPIRE",

abstract = "The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter, we use SPIRE observations of the galaxies M 99 and M 100 to explore the alternative approach of mapping the interstellar medium using the continuum emission from the dust. We have compared the methods by measuring the relationship between the star-formation rate and the surface density of gas in the galaxies using both methods. We find the two methods give relationships with a similar dispersion, confirming that observing the continuum emission from the dust is a promising method of mapping the interstellar medium in galaxies.",

keywords = "ISM: abundances, dust, extinction, galaxies: ISM, galaxies: spiral",

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

year = "2010",

doi = "10.1051/0004-6361/201014536",

language = "English",

volume = "518",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "4",

}

Eales, SA, Smith, MWL, Wilson, CD, Bendo, GJ, Cortese, L, Pohlen, M, Boselli, A, Gomez, HL, Auld, R, Baes, M, Barlow, MJ, Bock, JJ, Bradford, M, Buat, V, Castro-Rodríguez, N, Chanial, P, Charlot, S, Ciesla, L, Clements, DL, Cooray, A, Cormier, D, Davies, JI, Dwek, E, Elbaz, D, Galametz, M, Galliano, F, Gear, WK, Glenn, J, Griffin, M, Hony, S, Isaak, K, Levenson, LR, Lu, N, Madden, S, O'Halloran, B, Okumura, K, Oliver, S, Page, MJ, Panuzzo, P, Papageorgiou, A, Parkin, TJ, Pérez-Fournon, I, Rangwala, N, Rigby, EE, Rousse, H, Rykala, A, Sacchi, N, Sauvage, M, Schulz, B, Schirm, MRP, Spinoglio, L, Srinivasan, S, Stevens, JA, Symeonidis, M, Trichas, M, Vaccari, M, Vigroux, L, Wozniak, H, Wright, GS & Zeilinger, WW 2010, 'Mapping the interstellar medium in galaxies with Herschel*/SPIRE', Astronomy and Astrophysics, vol. 518, no. 4, L62. https://doi.org/10.1051/0004-6361/201014536

TY - JOUR

T1 - Mapping the interstellar medium in galaxies with Herschel*/SPIRE

AU - Eales, S. A.

AU - Smith, M. W.L.

AU - Wilson, C. D.

AU - Bendo, G. J.

AU - Cortese, L.

AU - Pohlen, M.

AU - Boselli, A.

AU - Gomez, H. L.

AU - Auld, R.

AU - Baes, M.

AU - Barlow, M. J.

AU - Bock, J. J.

AU - Bradford, M.

AU - Buat, V.

AU - Castro-Rodríguez, N.

AU - Chanial, P.

AU - Charlot, S.

AU - Ciesla, L.

AU - Clements, D. L.

AU - Cooray, A.

AU - Cormier, D.

AU - Davies, J. I.

AU - Dwek, E.

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.

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 - Pérez-Fournon, I.

AU - Rangwala, N.

AU - Rigby, E. E.

AU - Rousse, H.

AU - Rykala, A.

AU - Sacchi, N.

AU - Sauvage, M.

AU - Schulz, B.

AU - Schirm, M. R.P.

AU - Spinoglio, L.

AU - Srinivasan, S.

AU - Stevens, J. A.

AU - Symeonidis, M.

AU - Trichas, M.

AU - Vaccari, M.

AU - Vigroux, L.

AU - Wozniak, H.

AU - Wright, G. S.

AU - Zeilinger, W. W.

PY - 2010

Y1 - 2010

N2 - The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter, we use SPIRE observations of the galaxies M 99 and M 100 to explore the alternative approach of mapping the interstellar medium using the continuum emission from the dust. We have compared the methods by measuring the relationship between the star-formation rate and the surface density of gas in the galaxies using both methods. We find the two methods give relationships with a similar dispersion, confirming that observing the continuum emission from the dust is a promising method of mapping the interstellar medium in galaxies.

AB - The standard method of mapping the interstellar medium in a galaxy, by observing the molecular gas in the CO 1-0 line and the atomic gas in the 21-cm line, is largely limited with current telescopes to galaxies in the nearby universe. In this letter, we use SPIRE observations of the galaxies M 99 and M 100 to explore the alternative approach of mapping the interstellar medium using the continuum emission from the dust. We have compared the methods by measuring the relationship between the star-formation rate and the surface density of gas in the galaxies using both methods. We find the two methods give relationships with a similar dispersion, confirming that observing the continuum emission from the dust is a promising method of mapping the interstellar medium in galaxies.

KW - ISM: abundances

KW - dust, extinction

KW - galaxies: ISM

KW - galaxies: spiral

UR - https://www.scopus.com/pages/publications/77957813887

U2 - 10.1051/0004-6361/201014536

DO - 10.1051/0004-6361/201014536

M3 - Article

SN - 0004-6361

VL - 518

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 4

M1 - L62

ER -

Mapping the interstellar medium in galaxies with Herschel*/SPIRE

Abstract

UN SDGs

Keywords

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