The M51 MIR Spectral Cube: A "Rosetta Stone" for Galaxy Evolution

Other

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

The SINGS legacy survey is collecting a remarkable dataset for a large sample of nearby galaxies. Due to time constraints, however, the spectral data are limited. Except for the nucleus and a few selected HII regions, no SINGS galaxy has a full 5--37 micron spectral coverage across a galactic disk. The LL strips across the disks cover 14--37 microns missing most of the PAH features and other important spectral diagnostics limiting the use of the broadband data. This leaves open important questions about the state of the interstellar medium and the radial and regional variations across the disk. We propose to study the complete mid-infrared spectrum at low resolution (SL+LL) across the disk of the well studied, face-on, grand design spiral M51. We also propose to exploit the new peak-up imaging mode to obtain a 16 micron map of M51 to trace the dust continuum and determine the true PAH strengths. We chose M51 not only because it has a wealth of ancillary data but also because we have recently acquired a complete single dish + interferometer CO mosaic and 4, 6 and 20 cm radio continuum maps. This rare combination of data is well suited for a detailed study of the ISM as the CO traces the molecular gas and the radio continuum traces (extinction-free) star formation. We will combine these data with the proposed mid-infrared spectral data to determine the variations in the dust continuum and PAH emission as a function of radius and environment, the change in the ISM density, radiation field and grain size, and the change in the fraction of warm molecular gas across the disk. With this study M51 will be the spectral template for interpreting the wealth of broadband infrared data on nearby galaxies, and for improving our understanding of the dust content and dust properties of high redshift galaxies that are derived from rest-frame mid-infrared emission studies.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

The M51 MIR Spectral Cube: A "Rosetta Stone" for Galaxy Evolution does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The M51 MIR Spectral Cube: A "Rosetta Stone" for Galaxy Evolution, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The M51 MIR Spectral Cube: A "Rosetta Stone" for Galaxy Evolution will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1166880

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.