A CO isotopologue Line Atlas within the Whirlpool galaxy Survey (CLAWS)

• Published in: Astronomy and astrophysics (Berlin) 2022-06, Vol.662, p.A89
• Main Authors: den Brok, Jakob S., Bigiel, Frank, Sliwa, Kazimierz, Saito, Toshiki, Usero, Antonio, Schinnerer, Eva, Leroy, Adam K., Jiménez-Donaire, María J., Rosolowsky, Erik, Barnes, Ashley T., Puschnig, Johannes, Pety, Jérôme, Schruba, Andreas, Bešlić, Ivana, Cao, Yixian, Eibensteiner, Cosima, Glover, Simon C. O., Klessen, Ralf S., Diederik Kruijssen, J. M., Meidt, Sharon E., Neumann, Lukas, Tomičić, Neven, Pan, Hsi-An, Querejeta, Miguel, Watkins, Elizabeth, Williams, Thomas G., Wilner, David
• Format: Article
• Language: English
• Subjects: Astrophysics; Sciences of the Universe
• ISSN: 0004-6361; 1432-0746; 1432-0756
• DOI: 10.1051/0004-6361/202142247

We present the CO isotopologue Line Atlas within the Whirpool galaxy Survey (CLAWS), which is based on an IRAM 30 m large programme that provides a benchmark study of numerous faint CO isotopologues in the millimetre-wavelength regime across the full disc of the nearby grand-design spiral galaxy M 51 (NGC 5194). The survey’s core goal is to use the low- J CO isotopologue lines to constrain CO excitation and chemistry, and therefrom the local physical conditions of the gas. In this survey paper, we describe the CLAWS observing and data reduction strategies. We map the J = 1 → 0 and 2 → 1 transitions of the CO isotopologues 12 CO, 13 CO, C 18 O, and C 17 O, as well as several supplementary lines within the 1 mm and 3 mm window (CN(1-0), CS (2-1), CH 3 OH(2-1), N 2 H + (1–0), and HC 3 N (10–9)) at ~1 kpc resolution. A total observation time of 149 h offers unprecedented sensitivity. We use these data to explore several CO isotopologue line ratios in detail, study their radial (and azimuthal) trends, and investigate whether changes in line ratios stem from changes in interstellar medium properties such as gas temperatures, densities, or chemical abundances. For example, we find negative radial trends for the 13 CO/ 12 CO, C 18 O/ 12 CO, and C 18 O/ 13 CO line ratios in their J = 1 → 0 transitions. We also find variations with the local environment, such as higher 12 CO (2–1)/(1–0) or 13 CO/ 12 CO (1-0) line ratios in interarm regions compared to spiral arm regions. We propose that these aforementioned variations in CO line ratios are most likely due to a variation in the optical depth, though abundance variations due to selective nucleosynthesis on a galaxy-wide scale could also play a role. We also study the CO spectral line energy distribution (SLED) using archival JCMT 12 CO (3–2) data and find a variation in the SLED shape with local environmental parameters, suggesting changes in the optical depth, gas temperatures, or densities.