The Energy Budget of Massive Star-Formation in Andromeda

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

Scientific paper

M 31, the nearest massive galaxy, affords a unique opportunity to study the energy balance of the star-formation (SF) process on the spatial scales (<50 pc) of individual SF regions. For the `heating terms', UV to near-IR data from the Pan-chromatic Hubble Andromeda Treasury (PHAT) provide a direct census of all young stars in M 31; for the `cooling terms', we have compiled an unprecedented set of multi-wavelength data to trace the thermal state of ISM gas and dust across its multiple phases. This dataset includes far-IR and sub-mm broadband mapping across the whole disk of M 31 using the PACS and SPIRE instruments on Herschel to trace the dust spectral energy distribution; PACS spectroscopy in several regions of the key far-IR cooling lines--[CII] 158 μm and [OI] 63 μm --to trace the thermal state of neutral ISM gas; and fully-sampled optical integral-field spectroscopy from 3700-7100 Angstrom covering the same fields to probe the excitation and structure of ionized gas. The combination of these surveys will allow us to trace UV photons from their origin in massive stars through their various paths to heating ISM dust and gas. In this poster we present early results using the PACS and SPIRE photometry to study the heating of dust by different age stellar populations in the bulge and disk of M 31.

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 Energy Budget of Massive Star-Formation in Andromeda 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 Energy Budget of Massive Star-Formation in Andromeda, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Energy Budget of Massive Star-Formation in Andromeda will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1582223

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