Matches in SemOpenAlex for { <https://semopenalex.org/work/W2106992248> ?p ?o ?g. }
- W2106992248 endingPage "567" @default.
- W2106992248 startingPage "553" @default.
- W2106992248 abstract "Sharpless 170 is a diffuse Hii region ionized by a single main sequence O-star located near the periphery of a small dense molecular cloud at a distance of ~2 kpc. We describe wide-field observations of the region in the radio continuum, in Hi and CO-lines, and in the far-infrared which delineate the major ionized, atomic, molecular and dust components of the gas affected by the exciting star. From the thermal continuum emission we estimate the mass of ionized gas at ~350 within a radius of ~7 pc. The Hi (λ21 cm) and far-infrared observations show an extended low-density atomic component, of ~1000 , within an irregular boundary surrounding the ionized gas of mean radius ~10 pc. Mean densities in the Hi and Hii are similar, in the range 9–16 nucleons cm-3. CO emission shows a molecular cloud of ~1150 within an area 6 pc 4 pc with densities ~2000 nucleons cm-3. A compact infrared component coincides with the cloud. The exciting star is located on the near side of the cloud, just inside the southern periphery. Sh170 is an example of a young Hii region with the ionized gas, seen in Hα emission, streaming outward in the manner of a “champagne flow”. Although the observed velocities of the Hi are close to the mean velocity of the CO cloud, the morphology of the associated atomic hydrogen closely resembles that seen in the surrounds of other young Hii regions which show clear evidence of expansion of their Hi. We propose that much of the Hi is a diffuse dissociation zone beyond the ionization front, in directions from the star within a wide annulus, approximately transverse to the line-of-sight, between the dense photon-bounded region on the far side of the star and the density-bounded ionized flow region on the near side. In this view, much of the associated atomic gas, like the ionized gas, has been eroded from the molecular cloud in a small fraction (≤10%) of the star's main sequence lifetime." @default.
- W2106992248 created "2016-06-24" @default.
- W2106992248 creator A5006131794 @default.
- W2106992248 creator A5046025669 @default.
- W2106992248 creator A5057390630 @default.
- W2106992248 creator A5066974141 @default.
- W2106992248 date "2004-09-21" @default.
- W2106992248 modified "2023-09-27" @default.
- W2106992248 title "Sharpless 170 and the surrounding interstellar medium" @default.
- W2106992248 cites W105218988 @default.
- W2106992248 cites W1964203820 @default.
- W2106992248 cites W1967252168 @default.
- W2106992248 cites W1969747332 @default.
- W2106992248 cites W1975207394 @default.
- W2106992248 cites W1978425700 @default.
- W2106992248 cites W1979692684 @default.
- W2106992248 cites W1985189565 @default.
- W2106992248 cites W1995430022 @default.
- W2106992248 cites W2001661887 @default.
- W2106992248 cites W2001663399 @default.
- W2106992248 cites W2006669392 @default.
- W2106992248 cites W2006869439 @default.
- W2106992248 cites W2007839778 @default.
- W2106992248 cites W2007987053 @default.
- W2106992248 cites W2018870734 @default.
- W2106992248 cites W2019579421 @default.
- W2106992248 cites W2023409203 @default.
- W2106992248 cites W2039874334 @default.
- W2106992248 cites W2042802546 @default.
- W2106992248 cites W2044992590 @default.
- W2106992248 cites W2045487281 @default.
- W2106992248 cites W2052491072 @default.
- W2106992248 cites W2066286490 @default.
- W2106992248 cites W2086260412 @default.
- W2106992248 cites W2089469010 @default.
- W2106992248 cites W2152648017 @default.
- W2106992248 cites W2166075916 @default.
- W2106992248 cites W2169213604 @default.
- W2106992248 cites W2172351759 @default.
- W2106992248 cites W3121663239 @default.
- W2106992248 doi "https://doi.org/10.1051/0004-6361:20034352" @default.
- W2106992248 hasPublicationYear "2004" @default.
- W2106992248 type Work @default.
- W2106992248 sameAs 2106992248 @default.
- W2106992248 citedByCount "7" @default.
- W2106992248 countsByYear W21069922482012 @default.
- W2106992248 countsByYear W21069922482014 @default.
- W2106992248 countsByYear W21069922482020 @default.
- W2106992248 countsByYear W21069922482022 @default.
- W2106992248 crossrefType "journal-article" @default.
- W2106992248 hasAuthorship W2106992248A5006131794 @default.
- W2106992248 hasAuthorship W2106992248A5046025669 @default.
- W2106992248 hasAuthorship W2106992248A5057390630 @default.
- W2106992248 hasAuthorship W2106992248A5066974141 @default.
- W2106992248 hasBestOaLocation W21069922481 @default.
- W2106992248 hasConcept C121332964 @default.
- W2106992248 hasConcept C125857072 @default.
- W2106992248 hasConcept C1276947 @default.
- W2106992248 hasConcept C145148216 @default.
- W2106992248 hasConcept C150846664 @default.
- W2106992248 hasConcept C158355884 @default.
- W2106992248 hasConcept C178635117 @default.
- W2106992248 hasConcept C196939603 @default.
- W2106992248 hasConcept C198291218 @default.
- W2106992248 hasConcept C2778042268 @default.
- W2106992248 hasConcept C38652104 @default.
- W2106992248 hasConcept C41008148 @default.
- W2106992248 hasConcept C44870925 @default.
- W2106992248 hasConcept C62520636 @default.
- W2106992248 hasConcept C82706917 @default.
- W2106992248 hasConcept C86021447 @default.
- W2106992248 hasConcept C98444146 @default.
- W2106992248 hasConceptScore W2106992248C121332964 @default.
- W2106992248 hasConceptScore W2106992248C125857072 @default.
- W2106992248 hasConceptScore W2106992248C1276947 @default.
- W2106992248 hasConceptScore W2106992248C145148216 @default.
- W2106992248 hasConceptScore W2106992248C150846664 @default.
- W2106992248 hasConceptScore W2106992248C158355884 @default.
- W2106992248 hasConceptScore W2106992248C178635117 @default.
- W2106992248 hasConceptScore W2106992248C196939603 @default.
- W2106992248 hasConceptScore W2106992248C198291218 @default.
- W2106992248 hasConceptScore W2106992248C2778042268 @default.
- W2106992248 hasConceptScore W2106992248C38652104 @default.
- W2106992248 hasConceptScore W2106992248C41008148 @default.
- W2106992248 hasConceptScore W2106992248C44870925 @default.
- W2106992248 hasConceptScore W2106992248C62520636 @default.
- W2106992248 hasConceptScore W2106992248C82706917 @default.
- W2106992248 hasConceptScore W2106992248C86021447 @default.
- W2106992248 hasConceptScore W2106992248C98444146 @default.
- W2106992248 hasIssue "2" @default.
- W2106992248 hasLocation W21069922481 @default.
- W2106992248 hasLocation W21069922482 @default.
- W2106992248 hasOpenAccess W2106992248 @default.
- W2106992248 hasPrimaryLocation W21069922481 @default.
- W2106992248 hasRelatedWork W1662653051 @default.
- W2106992248 hasRelatedWork W1972160620 @default.
- W2106992248 hasRelatedWork W2017391605 @default.
- W2106992248 hasRelatedWork W2117510573 @default.