FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3102687792> ?p ?o ?g. }

• W3102687792 endingPage "147" @default.
• W3102687792 startingPage "147" @default.
• W3102687792 abstract "We present a new catalog of spectrophotometric distances and line of sight systemic velocities to 103 H ii regions between (longitude quadrants II and part of III). Two new velocities for each region are independently measured using 1 arcmin resolution 21 cm H i and 2.6 mm 12CO line maps (from the Canadian Galactic Plane Survey and Five College Radio Astronomy Observatory Outer Galaxy Surveys) that show where gaseous shells are observed around the periphery of the ionized gas. Known and neighboring O- and B-type stars with published UBV photometry and MK classifications are overlaid onto 21 cm continuum maps, and those stars observed within the boundary of the H ii emission (and whose distance is not more than three times the standard deviation of the others) are used to calculate new mean stellar distances to each of the 103 nebulae. Using this approach of excluding distance outliers from the mean distance to a group of many stars in each H ii region lessens the impact of anomalous reddening for certain individuals. The standard deviation of individual stellar distances in a cluster is typically 20% per stellar distance, and the error in the mean distance to the cluster is typically ±10%. Final mean distances of nine common objects with very long baseline interferometry parallax distances show a 1:1 correspondence. Further, comparison with previous catalogs of H ii regions in these quadrants shows a 50% reduction in scatter for the distance to Perseus spiral arm objects in the same region, and a reduction by ∼1/ in scatter around a common angular velocity relative to the Sun (km s−1 kpc−1). The purpose of the catalog is to provide a foundation for more detailed large-scale Galactic spiral structure and dynamics (rotation curve, density wave streaming) studies in the 2nd and 3rd quadrants, which from the Sun's location is the most favorably viewed section of the Galaxy." @default.
• W3102687792 created "2020-11-23" @default.
• W3102687792 creator A5029887975 @default.
• W3102687792 creator A5054946106 @default.
• W3102687792 date "2015-10-14" @default.
• W3102687792 modified "2023-10-13" @default.
• W3102687792 title "A CGPS LOOK AT THE SPIRAL STRUCTURE OF THE OUTER MILKY WAY. I. DISTANCES AND VELOCITIES TO STAR-FORMING REGIONS" @default.
• W3102687792 cites W1972327829 @default.
• W3102687792 cites W1974167268 @default.
• W3102687792 cites W1976139832 @default.
• W3102687792 cites W1980145009 @default.
• W3102687792 cites W1981385557 @default.
• W3102687792 cites W1981860095 @default.
• W3102687792 cites W1984373204 @default.
• W3102687792 cites W1985758103 @default.
• W3102687792 cites W1993960902 @default.
• W3102687792 cites W2001661887 @default.
• W3102687792 cites W2001977925 @default.
• W3102687792 cites W2003751401 @default.
• W3102687792 cites W2005585394 @default.
• W3102687792 cites W2006669392 @default.
• W3102687792 cites W2006706874 @default.
• W3102687792 cites W2007897349 @default.
• W3102687792 cites W2015322641 @default.
• W3102687792 cites W2017721755 @default.
• W3102687792 cites W2019060208 @default.
• W3102687792 cites W2023382730 @default.
• W3102687792 cites W2023409203 @default.
• W3102687792 cites W2029623000 @default.
• W3102687792 cites W2050372348 @default.
• W3102687792 cites W2055623336 @default.
• W3102687792 cites W2057310326 @default.
• W3102687792 cites W2057634812 @default.
• W3102687792 cites W2061562494 @default.
• W3102687792 cites W2061634416 @default.
• W3102687792 cites W2069523339 @default.
• W3102687792 cites W2071791978 @default.
• W3102687792 cites W2074582833 @default.
• W3102687792 cites W2075644342 @default.
• W3102687792 cites W2131988517 @default.
• W3102687792 cites W2137112804 @default.
• W3102687792 cites W2152648017 @default.
• W3102687792 cites W2168207996 @default.
• W3102687792 cites W2259968672 @default.
• W3102687792 cites W3098218194 @default.
• W3102687792 cites W3099217402 @default.
• W3102687792 cites W3099571084 @default.
• W3102687792 cites W3099830973 @default.
• W3102687792 cites W3101536651 @default.
• W3102687792 cites W3101967518 @default.
• W3102687792 cites W3102615369 @default.
• W3102687792 cites W3103664646 @default.
• W3102687792 cites W3105047641 @default.
• W3102687792 cites W3105883850 @default.
• W3102687792 cites W4300592832 @default.
• W3102687792 doi "https://doi.org/10.1088/0004-6256/150/5/147" @default.
• W3102687792 hasPublicationYear "2015" @default.
• W3102687792 type Work @default.
• W3102687792 sameAs 3102687792 @default.
• W3102687792 citedByCount "41" @default.
• W3102687792 countsByYear W31026877922015 @default.
• W3102687792 countsByYear W31026877922016 @default.
• W3102687792 countsByYear W31026877922017 @default.
• W3102687792 countsByYear W31026877922018 @default.
• W3102687792 countsByYear W31026877922019 @default.
• W3102687792 countsByYear W31026877922020 @default.
• W3102687792 countsByYear W31026877922021 @default.
• W3102687792 countsByYear W31026877922022 @default.
• W3102687792 countsByYear W31026877922023 @default.
• W3102687792 crossrefType "journal-article" @default.
• W3102687792 hasAuthorship W3102687792A5029887975 @default.
• W3102687792 hasAuthorship W3102687792A5054946106 @default.
• W3102687792 hasBestOaLocation W31026877921 @default.
• W3102687792 hasConcept C105795698 @default.
• W3102687792 hasConcept C121332964 @default.
• W3102687792 hasConcept C1276947 @default.
• W3102687792 hasConcept C133725777 @default.
• W3102687792 hasConcept C150846664 @default.
• W3102687792 hasConcept C183582522 @default.
• W3102687792 hasConcept C22679943 @default.
• W3102687792 hasConcept C33923547 @default.
• W3102687792 hasConcept C44870925 @default.
• W3102687792 hasConcept C52348108 @default.
• W3102687792 hasConcept C555520305 @default.
• W3102687792 hasConcept C63585750 @default.
• W3102687792 hasConcept C68271606 @default.
• W3102687792 hasConcept C98444146 @default.
• W3102687792 hasConceptScore W3102687792C105795698 @default.
• W3102687792 hasConceptScore W3102687792C121332964 @default.
• W3102687792 hasConceptScore W3102687792C1276947 @default.
• W3102687792 hasConceptScore W3102687792C133725777 @default.
• W3102687792 hasConceptScore W3102687792C150846664 @default.
• W3102687792 hasConceptScore W3102687792C183582522 @default.
• W3102687792 hasConceptScore W3102687792C22679943 @default.
• W3102687792 hasConceptScore W3102687792C33923547 @default.
• W3102687792 hasConceptScore W3102687792C44870925 @default.
• W3102687792 hasConceptScore W3102687792C52348108 @default.
• W3102687792 hasConceptScore W3102687792C555520305 @default.

• next