- Author
- GJ Bendo, CD Wilson, M Pohlen, M Sauvage, R Auld, Maarten Baes (UGent) , MJ Barlow, JJ Bock, A Boselli, M Bradford, V Buat, N Castro-Rodriguez, P Chanial, S Charlot, L Ciesla, DL Clements, A Cooray, D Cormier, L Cortese, JI Davies, E Dwek, SA Eales, D Elbaz, M Galametz, F Galliano, WK Gear, J Glenn, HL Gomez, M Griffin, S Hony, KG Isaak, LR Levenson, N Lu, S Madden, B O'Halloran, K Okumura, S Oliver, MJ Page, P Panuzzo, A Papageorgiou, TJ Parkin, I Perez-Fournon, N Rangwala, EE Rigby, H Roussel, A Rykala, N Sacchi, B Schulz, MRP Schirm, MWL Smith, L Spinoglio, JA Stevens, S Sundar, M Symeonidis, M Trichas, M Vaccari, L Vigroux, H Wozniak, GS Wright and WW Zeilinger
- Organization
- Abstract
- We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 mu m in the nearby spiral galaxy M81. We find that the ratios of wave bands between 160 and 500 mu m are primarily dependent on radius but that the ratio of 70 to 160 mu m emission shows no clear dependence on surface brightness or radius. These results along with analyses of the spectral energy distributions imply that the 160-500 mu m emission traces 15-30 K dust heated by evolved stars in the bulge and disc whereas the 70 mu m emission includes dust heated by the active galactic nucleus and young stars in star forming regions.
- Keywords
- galaxies: ISM, galaxies: spiral, galaxies: individual: M81, STAR-FORMATION RATES, H-ALPHA, GALAXIES, TELESCOPE, EMISSION, SPITZER, THINGS, FIELD
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Citation
Please use this url to cite or link to this publication: http://hdl.handle.net/1854/LU-1237201
- MLA
- Bendo, GJ, et al. “The Herschel Space Observatory View of Dust in M81.” ASTRONOMY & ASTROPHYSICS, vol. 518, 2010, doi:10.1051/0004-6361/201014568.
- APA
- Bendo, G., Wilson, C., Pohlen, M., Sauvage, M., Auld, R., Baes, M., … Zeilinger, W. (2010). The Herschel Space Observatory view of dust in M81. ASTRONOMY & ASTROPHYSICS, 518. https://doi.org/10.1051/0004-6361/201014568
- Chicago author-date
- Bendo, GJ, CD Wilson, M Pohlen, M Sauvage, R Auld, Maarten Baes, MJ Barlow, et al. 2010. “The Herschel Space Observatory View of Dust in M81.” ASTRONOMY & ASTROPHYSICS 518. https://doi.org/10.1051/0004-6361/201014568.
- Chicago author-date (all authors)
- Bendo, GJ, CD Wilson, M Pohlen, M Sauvage, R Auld, Maarten Baes, MJ Barlow, JJ Bock, A Boselli, M Bradford, V Buat, N Castro-Rodriguez, P Chanial, S Charlot, L Ciesla, DL Clements, A Cooray, D Cormier, L Cortese, JI Davies, E Dwek, SA Eales, D Elbaz, M Galametz, F Galliano, WK Gear, J Glenn, HL Gomez, M Griffin, S Hony, KG Isaak, LR Levenson, N Lu, S Madden, B O’Halloran, K Okumura, S Oliver, MJ Page, P Panuzzo, A Papageorgiou, TJ Parkin, I Perez-Fournon, N Rangwala, EE Rigby, H Roussel, A Rykala, N Sacchi, B Schulz, MRP Schirm, MWL Smith, L Spinoglio, JA Stevens, S Sundar, M Symeonidis, M Trichas, M Vaccari, L Vigroux, H Wozniak, GS Wright, and WW Zeilinger. 2010. “The Herschel Space Observatory View of Dust in M81.” ASTRONOMY & ASTROPHYSICS 518. doi:10.1051/0004-6361/201014568.
- Vancouver
- 1.Bendo G, Wilson C, Pohlen M, Sauvage M, Auld R, Baes M, et al. The Herschel Space Observatory view of dust in M81. ASTRONOMY & ASTROPHYSICS. 2010;518.
- IEEE
- [1]G. Bendo et al., “The Herschel Space Observatory view of dust in M81,” ASTRONOMY & ASTROPHYSICS, vol. 518, 2010.
@article{1237201, abstract = {{We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70-500 mu m in the nearby spiral galaxy M81. We find that the ratios of wave bands between 160 and 500 mu m are primarily dependent on radius but that the ratio of 70 to 160 mu m emission shows no clear dependence on surface brightness or radius. These results along with analyses of the spectral energy distributions imply that the 160-500 mu m emission traces 15-30 K dust heated by evolved stars in the bulge and disc whereas the 70 mu m emission includes dust heated by the active galactic nucleus and young stars in star forming regions.}}, articleno = {{L65}}, author = {{Bendo, GJ and Wilson, CD and Pohlen, M and Sauvage, M and Auld, R and Baes, Maarten and Barlow, MJ and Bock, JJ and Boselli, A and Bradford, M and Buat, V and Castro-Rodriguez, N and Chanial, P and Charlot, S and Ciesla, L and Clements, DL and Cooray, A and Cormier, D and Cortese, L and Davies, JI and Dwek, E and Eales, SA and Elbaz, D and Galametz, M and Galliano, F and Gear, WK and Glenn, J and Gomez, HL 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 Schulz, B and Schirm, MRP and Smith, MWL and Spinoglio, L and Stevens, JA and Sundar, S and Symeonidis, M and Trichas, M and Vaccari, M and Vigroux, L and Wozniak, H and Wright, GS and Zeilinger, WW}}, issn = {{0004-6361}}, journal = {{ASTRONOMY & ASTROPHYSICS}}, keywords = {{galaxies: ISM,galaxies: spiral,galaxies: individual: M81,STAR-FORMATION RATES,H-ALPHA,GALAXIES,TELESCOPE,EMISSION,SPITZER,THINGS,FIELD}}, language = {{eng}}, pages = {{4}}, title = {{The Herschel Space Observatory view of dust in M81}}, url = {{http://doi.org/10.1051/0004-6361/201014568}}, volume = {{518}}, year = {{2010}}, }
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