Matches in SemOpenAlex for { <https://semopenalex.org/work/W2093181503> ?p ?o ?g. }
- W2093181503 endingPage "42" @default.
- W2093181503 startingPage "42" @default.
- W2093181503 abstract "The Plateau de Bure Interferometer Arcsecond Whirlpool Survey has mapped the molecular gas in the central ∼9 kpc of M51 in its 12CO(1–0) line emission at a cloud-scale resolution of ∼40 pc using both IRAM telescopes. We utilize this data set to quantitatively characterize the relation of molecular gas (or CO emission) to other tracers of the interstellar medium, star formation, and stellar populations of varying ages. Using two-dimensional maps, a polar cross-correlation technique and pixel-by-pixel diagrams, we find: (1) that (as expected) the distribution of the molecular gas can be linked to different components of the gravitational potential; (2) evidence for a physical link between CO line emission and radio continuum that seems not to be caused by massive stars, but rather depends on the gas density; (3) a close spatial relation between polycyclic aromatic hydrocarbon (PAH) and molecular gas emission, but no predictive power of PAH emission for the molecular gas mass; (4) that the I − H color map is an excellent predictor of the distribution (and to a lesser degree, the brightness) of CO emission; and (5) that the impact of massive (UV-intense) young star-forming regions on the bulk of the molecular gas in central ∼9 kpc cannot be significant due to a complex spatial relation between molecular gas and star-forming regions that ranges from cospatial to spatially offset to absent. The last point, in particular, highlights the importance of galactic environment—and thus the underlying gravitational potential—for the distribution of molecular gas and star formation." @default.
- W2093181503 created "2016-06-24" @default.
- W2093181503 creator A5005870132 @default.
- W2093181503 creator A5011885853 @default.
- W2093181503 creator A5015636843 @default.
- W2093181503 creator A5031028129 @default.
- W2093181503 creator A5041571952 @default.
- W2093181503 creator A5046177229 @default.
- W2093181503 creator A5048954635 @default.
- W2093181503 creator A5057861867 @default.
- W2093181503 creator A5061165927 @default.
- W2093181503 creator A5061231234 @default.
- W2093181503 creator A5063633367 @default.
- W2093181503 creator A5085225449 @default.
- W2093181503 creator A5091551312 @default.
- W2093181503 date "2013-11-25" @default.
- W2093181503 modified "2023-10-12" @default.
- W2093181503 title "THE PdBI ARCSECOND WHIRLPOOL SURVEY (PAWS). I. A CLOUD-SCALE/MULTI-WAVELENGTH VIEW OF THE INTERSTELLAR MEDIUM IN A GRAND-DESIGN SPIRAL GALAXY" @default.
- W2093181503 cites W1507716615 @default.
- W2093181503 cites W1618003760 @default.
- W2093181503 cites W1681286495 @default.
- W2093181503 cites W1851199749 @default.
- W2093181503 cites W1911357967 @default.
- W2093181503 cites W1964187543 @default.
- W2093181503 cites W1964540854 @default.
- W2093181503 cites W1966185800 @default.
- W2093181503 cites W1970084939 @default.
- W2093181503 cites W1970659039 @default.
- W2093181503 cites W1973465889 @default.
- W2093181503 cites W1976879631 @default.
- W2093181503 cites W1977521416 @default.
- W2093181503 cites W1978342063 @default.
- W2093181503 cites W1980064171 @default.
- W2093181503 cites W1982889622 @default.
- W2093181503 cites W1983818684 @default.
- W2093181503 cites W1987704721 @default.
- W2093181503 cites W1988332339 @default.
- W2093181503 cites W1989735293 @default.
- W2093181503 cites W1991391334 @default.
- W2093181503 cites W1992936976 @default.
- W2093181503 cites W1993230081 @default.
- W2093181503 cites W1993519651 @default.
- W2093181503 cites W1995435934 @default.
- W2093181503 cites W1997972076 @default.
- W2093181503 cites W1998035806 @default.
- W2093181503 cites W1998762398 @default.
- W2093181503 cites W1999530467 @default.
- W2093181503 cites W1999691522 @default.
- W2093181503 cites W2000257287 @default.
- W2093181503 cites W2001650506 @default.
- W2093181503 cites W2003637061 @default.
- W2093181503 cites W2006878995 @default.
- W2093181503 cites W2009019383 @default.
- W2093181503 cites W2010622696 @default.
- W2093181503 cites W2014555677 @default.
- W2093181503 cites W2015761844 @default.
- W2093181503 cites W2017066555 @default.
- W2093181503 cites W2018489616 @default.
- W2093181503 cites W2019579421 @default.
- W2093181503 cites W2020170218 @default.
- W2093181503 cites W2023184232 @default.
- W2093181503 cites W2023793647 @default.
- W2093181503 cites W2024821919 @default.
- W2093181503 cites W2026067008 @default.
- W2093181503 cites W2026328109 @default.
- W2093181503 cites W2032202691 @default.
- W2093181503 cites W2032832347 @default.
- W2093181503 cites W2037131602 @default.
- W2093181503 cites W2040364743 @default.
- W2093181503 cites W2042240341 @default.
- W2093181503 cites W2046271943 @default.
- W2093181503 cites W2046523578 @default.
- W2093181503 cites W2047682423 @default.
- W2093181503 cites W2048274049 @default.
- W2093181503 cites W2052629426 @default.
- W2093181503 cites W2056753473 @default.
- W2093181503 cites W2058731249 @default.
- W2093181503 cites W2059907540 @default.
- W2093181503 cites W2061391030 @default.
- W2093181503 cites W2061531105 @default.
- W2093181503 cites W2063375458 @default.
- W2093181503 cites W2063395797 @default.
- W2093181503 cites W2063505240 @default.
- W2093181503 cites W2066948687 @default.
- W2093181503 cites W2067062904 @default.
- W2093181503 cites W2067542394 @default.
- W2093181503 cites W2069143761 @default.
- W2093181503 cites W2070202907 @default.
- W2093181503 cites W2070444660 @default.
- W2093181503 cites W2070850663 @default.
- W2093181503 cites W2074529843 @default.
- W2093181503 cites W2076064009 @default.
- W2093181503 cites W2076783262 @default.
- W2093181503 cites W2078001023 @default.
- W2093181503 cites W2078583702 @default.
- W2093181503 cites W2079264260 @default.
- W2093181503 cites W2081595008 @default.
- W2093181503 cites W2085053169 @default.