In:
The Astrophysical Journal, American Astronomical Society, Vol. 925, No. 1 ( 2022-01-01), p. 59-
Kurzfassung:
Molecular emission was imaged with ALMA from numerous components near and within bright H 2 -emitting knots and absorbing dust globules in the Crab Nebula. These observations provide a critical test of how energetic photons and particles produced in a young supernova remnant interact with gas, cleanly differentiating between competing models. The four fields targeted show contrasting properties but within them, seventeen distinct molecular clouds are identified with CO emission; a few also show emission from HCO + , SiO, and/or SO. These observations are compared with Cloudy models of these knots. It has been suggested that the Crab filaments present an exotic environment in which H 2 emission comes from a mostly neutral zone probably heated by cosmic rays produced in the supernova surrounding a cool core of molecular gas. Our model is consistent with the observed CO J = 3 − 2 line strength. These molecular line emitting knots in the Crab Nebula present a novel phase of the ISM representative of many important astrophysical environments.
Materialart:
Online-Ressource
ISSN:
0004-637X
,
1538-4357
DOI:
10.3847/1538-4357/ac391a
Sprache:
Unbekannt
Verlag:
American Astronomical Society
Publikationsdatum:
2022
ZDB Id:
2207648-7
ZDB Id:
1473835-1
SSG:
16,12
