We measure the CO-to-H2conversion factor (
We present an analysis of nearly 1000 near-infrared, integrated-light spectra from APOGEE in the inner ∼7 kpc of M31. We utilize full-spectrum fitting with A-LIST simple stellar population spectral templates that represent a population of stars with the same age, [M/H], and [
- Award ID(s):
- 1911129
- NSF-PAR ID:
- 10431913
- Publisher / Repository:
- DOI PREFIX: 10.3847
- Date Published:
- Journal Name:
- The Astrophysical Journal
- Volume:
- 952
- Issue:
- 1
- ISSN:
- 0004-637X
- Format(s):
- Medium: X Size: Article No. 23
- Size(s):
- ["Article No. 23"]
- Sponsoring Org:
- National Science Foundation
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