FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3101931036> ?p ?o ?g. }

• W3101931036 endingPage "25" @default.
• W3101931036 startingPage "25" @default.
• W3101931036 abstract "The presence of a well-defined and narrow dust lane in an edge-on spiral galaxy is the observational signature of a thin and dense molecular disk, in which gravitational collapse has overcome turbulence. Using a sample of galaxies out to z ∼ 1 extracted from the COSMOS survey, we identify the fraction of massive (L*V) disks that display a dust lane. Our goal is to explore the evolution in the stability of the molecular interstellar medium (ISM) disks in spiral galaxies over a cosmic timescale. We check the reliability of our morphological classifications against changes in rest-frame wavelength, resolution, and cosmic dimming with (artificially redshifted) images of local galaxies from the Sloan Digital Sky Survey. We find that the fraction of L*V disks with dust lanes in COSMOS is consistent with the local fraction (≈80%) out to z ∼ 0.7. At z = 0.8, the dust lane fraction is only slightly lower. A somewhat lower dust lane fraction in starbursting galaxies tentatively supports the notion that a high specific star formation rate can efficiently destroy or inhibit a dense molecular disk. A small subsample of higher redshift COSMOS galaxies display low internal reddening (E[B − V]), as well as a low incidence of dust lanes. These may be disks in which the growth of the dusty ISM disk lags behind that of the stellar disk. We note that at z = 0.8, the most massive galaxies display a lower dust lane fraction than lower mass galaxies. A small contribution of recent mergers or starbursts to this most massive population may be responsible. The fact that the fraction of galaxies with dust lanes in COSMOS is consistent with little or no evolution implies that models to explain the spectral energy distribution or the host galaxy dust extinction of supernovae based on local galaxies are still applicable to higher redshift spirals. It also suggests that dust lanes are long-lived phenomena or can be reformed over very short timescales." @default.
• W3101931036 created "2020-11-23" @default.
• W3101931036 creator A5026833343 @default.
• W3101931036 creator A5043083140 @default.
• W3101931036 creator A5045088665 @default.
• W3101931036 creator A5051126966 @default.
• W3101931036 creator A5052208759 @default.
• W3101931036 creator A5058865181 @default.
• W3101931036 creator A5078864354 @default.
• W3101931036 creator A5083249765 @default.
• W3101931036 date "2012-06-12" @default.
• W3101931036 modified "2023-10-16" @default.
• W3101931036 title "EVOLUTION IN THE DUST LANE FRACTION OF EDGE-ON<i>L</i>*_<i>V</i>SPIRAL GALAXIES SINCE<i>z</i>= 0.8" @default.
• W3101931036 cites W1970196846 @default.
• W3101931036 cites W1987341110 @default.
• W3101931036 cites W1989649987 @default.
• W3101931036 cites W1990479252 @default.
• W3101931036 cites W1991586413 @default.
• W3101931036 cites W1992923622 @default.
• W3101931036 cites W2018828554 @default.
• W3101931036 cites W2040277629 @default.
• W3101931036 cites W2043714894 @default.
• W3101931036 cites W2053781585 @default.
• W3101931036 cites W2068078315 @default.
• W3101931036 cites W2130225077 @default.
• W3101931036 cites W2168500673 @default.
• W3101931036 cites W2524672347 @default.
• W3101931036 cites W3043574796 @default.
• W3101931036 cites W3100376715 @default.
• W3101931036 cites W3103454316 @default.
• W3101931036 cites W3105003657 @default.
• W3101931036 cites W3149990775 @default.
• W3101931036 doi "https://doi.org/10.1088/0004-637x/753/1/25" @default.
• W3101931036 hasPublicationYear "2012" @default.
• W3101931036 type Work @default.
• W3101931036 sameAs 3101931036 @default.
• W3101931036 citedByCount "10" @default.
• W3101931036 countsByYear W31019310362013 @default.
• W3101931036 countsByYear W31019310362014 @default.
• W3101931036 countsByYear W31019310362015 @default.
• W3101931036 countsByYear W31019310362017 @default.
• W3101931036 countsByYear W31019310362019 @default.
• W3101931036 countsByYear W31019310362021 @default.
• W3101931036 countsByYear W31019310362022 @default.
• W3101931036 countsByYear W31019310362023 @default.
• W3101931036 crossrefType "journal-article" @default.
• W3101931036 hasAuthorship W3101931036A5026833343 @default.
• W3101931036 hasAuthorship W3101931036A5043083140 @default.
• W3101931036 hasAuthorship W3101931036A5045088665 @default.
• W3101931036 hasAuthorship W3101931036A5051126966 @default.
• W3101931036 hasAuthorship W3101931036A5052208759 @default.
• W3101931036 hasAuthorship W3101931036A5058865181 @default.
• W3101931036 hasAuthorship W3101931036A5078864354 @default.
• W3101931036 hasAuthorship W3101931036A5083249765 @default.
• W3101931036 hasBestOaLocation W31019310361 @default.
• W3101931036 hasConcept C121332964 @default.
• W3101931036 hasConcept C125857072 @default.
• W3101931036 hasConcept C1276947 @default.
• W3101931036 hasConcept C132645408 @default.
• W3101931036 hasConcept C168589115 @default.
• W3101931036 hasConcept C196939603 @default.
• W3101931036 hasConcept C33024259 @default.
• W3101931036 hasConcept C44870925 @default.
• W3101931036 hasConcept C63585750 @default.
• W3101931036 hasConcept C98444146 @default.
• W3101931036 hasConceptScore W3101931036C121332964 @default.
• W3101931036 hasConceptScore W3101931036C125857072 @default.
• W3101931036 hasConceptScore W3101931036C1276947 @default.
• W3101931036 hasConceptScore W3101931036C132645408 @default.
• W3101931036 hasConceptScore W3101931036C168589115 @default.
• W3101931036 hasConceptScore W3101931036C196939603 @default.
• W3101931036 hasConceptScore W3101931036C33024259 @default.
• W3101931036 hasConceptScore W3101931036C44870925 @default.
• W3101931036 hasConceptScore W3101931036C63585750 @default.
• W3101931036 hasConceptScore W3101931036C98444146 @default.
• W3101931036 hasIssue "1" @default.
• W3101931036 hasLocation W31019310361 @default.
• W3101931036 hasLocation W31019310362 @default.
• W3101931036 hasOpenAccess W3101931036 @default.
• W3101931036 hasPrimaryLocation W31019310361 @default.
• W3101931036 hasRelatedWork W1981635330 @default.
• W3101931036 hasRelatedWork W2060449082 @default.
• W3101931036 hasRelatedWork W2089107762 @default.
• W3101931036 hasRelatedWork W2094340834 @default.
• W3101931036 hasRelatedWork W2096624375 @default.
• W3101931036 hasRelatedWork W3098742842 @default.
• W3101931036 hasRelatedWork W3100685542 @default.
• W3101931036 hasRelatedWork W3121549445 @default.
• W3101931036 hasRelatedWork W3168417647 @default.
• W3101931036 hasRelatedWork W4292503076 @default.
• W3101931036 hasVolume "753" @default.
• W3101931036 isParatext "false" @default.
• W3101931036 isRetracted "false" @default.
• W3101931036 magId "3101931036" @default.
• W3101931036 workType "article" @default.