FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1975694125> ?p ?o ?g. }

• W1975694125 endingPage "1222" @default.
• W1975694125 startingPage "1209" @default.
• W1975694125 abstract "We combine new observations from the Hubble Space Telescope's Advanced Camera of Survey with existing data to investigate the wavelength dependence of near-IR (NIR) extinction. Previous studies suggest a power law form for NIR extinction, with a universal value of the exponent, although some recent observations indicate that significant sight line-to-sight line variability may exist. We show that a power-law model for the NIR extinction provides an excellent fit to most extinction curves, but that the value of the power, β, varies significantly from sight line to sight line. Therefore, it seems that a universal NIR extinction law is not possible. Instead, we find that as β decreases, R(V) ≡ A(V)/E(B − V) tends to increase, suggesting that NIR extinction curves which have been considered peculiar may, in fact, be typical for different R(V) values. We show that the power-law parameters can depend on the wavelength interval used to derive them, with the β increasing as longer wavelengths are included. This result implies that extrapolating power-law fits to determine R(V) is unreliable. To avoid this problem, we adopt a different functional form for NIR extinction. This new form mimics a power law whose exponent increases with wavelength, has only two free parameters, can fit all of our curves over a longer wavelength baseline and to higher precision, and produces R(V) values which are consistent with independent estimates and commonly used methods for estimating R(V). Furthermore, unlike the power-law model, it gives R(V)s that are independent of the wavelength interval used to derive them. It also suggests that the relation can estimate R(V) to ±0.12. Finally, we use model extinction curves to show that our extinction curves are in accord with theoretical expectations, and demonstrate how large samples of observational quantities can provide useful constraints on the grain properties." @default.
• W1975694125 created "2016-06-24" @default.
• W1975694125 creator A5059798421 @default.
• W1975694125 creator A5086548160 @default.
• W1975694125 date "2009-06-19" @default.
• W1975694125 modified "2023-09-27" @default.
• W1975694125 title "AN ANALYSIS OF THE SHAPES OF INTERSTELLAR EXTINCTION CURVES. VI. THE NEAR-IR EXTINCTION LAW" @default.
• W1975694125 cites W1965372241 @default.
• W1975694125 cites W1967340141 @default.
• W1975694125 cites W1974394716 @default.
• W1975694125 cites W1989940292 @default.
• W1975694125 cites W1999735742 @default.
• W1975694125 cites W2012118736 @default.
• W1975694125 cites W2012853668 @default.
• W1975694125 cites W2018256249 @default.
• W1975694125 cites W2032764027 @default.
• W1975694125 cites W2035198704 @default.
• W1975694125 cites W2039907165 @default.
• W1975694125 cites W2040657662 @default.
• W1975694125 cites W2051217514 @default.
• W1975694125 cites W2060447404 @default.
• W1975694125 cites W2071708155 @default.
• W1975694125 cites W2083264490 @default.
• W1975694125 cites W2089167229 @default.
• W1975694125 cites W2096655197 @default.
• W1975694125 cites W2114246636 @default.
• W1975694125 cites W2148504537 @default.
• W1975694125 cites W2167635287 @default.
• W1975694125 cites W3100911840 @default.
• W1975694125 cites W3104052455 @default.
• W1975694125 cites W3105592386 @default.
• W1975694125 cites W3105883850 @default.
• W1975694125 cites W3124358277 @default.
• W1975694125 doi "https://doi.org/10.1088/0004-637x/699/2/1209" @default.
• W1975694125 hasPublicationYear "2009" @default.
• W1975694125 type Work @default.
• W1975694125 sameAs 1975694125 @default.
• W1975694125 citedByCount "99" @default.
• W1975694125 countsByYear W19756941252012 @default.
• W1975694125 countsByYear W19756941252013 @default.
• W1975694125 countsByYear W19756941252014 @default.
• W1975694125 countsByYear W19756941252015 @default.
• W1975694125 countsByYear W19756941252016 @default.
• W1975694125 countsByYear W19756941252017 @default.
• W1975694125 countsByYear W19756941252018 @default.
• W1975694125 countsByYear W19756941252019 @default.
• W1975694125 countsByYear W19756941252020 @default.
• W1975694125 countsByYear W19756941252021 @default.
• W1975694125 countsByYear W19756941252022 @default.
• W1975694125 countsByYear W19756941252023 @default.
• W1975694125 crossrefType "journal-article" @default.
• W1975694125 hasAuthorship W1975694125A5059798421 @default.
• W1975694125 hasAuthorship W1975694125A5086548160 @default.
• W1975694125 hasBestOaLocation W19756941251 @default.
• W1975694125 hasConcept C101991246 @default.
• W1975694125 hasConcept C105795698 @default.
• W1975694125 hasConcept C120665830 @default.
• W1975694125 hasConcept C121332964 @default.
• W1975694125 hasConcept C138885662 @default.
• W1975694125 hasConcept C17744445 @default.
• W1975694125 hasConcept C198352243 @default.
• W1975694125 hasConcept C199539241 @default.
• W1975694125 hasConcept C2524010 @default.
• W1975694125 hasConcept C2780388253 @default.
• W1975694125 hasConcept C2780928442 @default.
• W1975694125 hasConcept C33923547 @default.
• W1975694125 hasConcept C41895202 @default.
• W1975694125 hasConcept C44870925 @default.
• W1975694125 hasConcept C6260449 @default.
• W1975694125 hasConcept C87040749 @default.
• W1975694125 hasConceptScore W1975694125C101991246 @default.
• W1975694125 hasConceptScore W1975694125C105795698 @default.
• W1975694125 hasConceptScore W1975694125C120665830 @default.
• W1975694125 hasConceptScore W1975694125C121332964 @default.
• W1975694125 hasConceptScore W1975694125C138885662 @default.
• W1975694125 hasConceptScore W1975694125C17744445 @default.
• W1975694125 hasConceptScore W1975694125C198352243 @default.
• W1975694125 hasConceptScore W1975694125C199539241 @default.
• W1975694125 hasConceptScore W1975694125C2524010 @default.
• W1975694125 hasConceptScore W1975694125C2780388253 @default.
• W1975694125 hasConceptScore W1975694125C2780928442 @default.
• W1975694125 hasConceptScore W1975694125C33923547 @default.
• W1975694125 hasConceptScore W1975694125C41895202 @default.
• W1975694125 hasConceptScore W1975694125C44870925 @default.
• W1975694125 hasConceptScore W1975694125C6260449 @default.
• W1975694125 hasConceptScore W1975694125C87040749 @default.
• W1975694125 hasIssue "2" @default.
• W1975694125 hasLocation W19756941251 @default.
• W1975694125 hasLocation W19756941252 @default.
• W1975694125 hasOpenAccess W1975694125 @default.
• W1975694125 hasPrimaryLocation W19756941251 @default.
• W1975694125 hasRelatedWork W2017751841 @default.
• W1975694125 hasRelatedWork W2050632788 @default.
• W1975694125 hasRelatedWork W2053446678 @default.
• W1975694125 hasRelatedWork W2169393734 @default.
• W1975694125 hasRelatedWork W2795003752 @default.
• W1975694125 hasRelatedWork W3070256043 @default.
• W1975694125 hasRelatedWork W3092852006 @default.

• next