Emai's Variable Coding of Adjuncts

Schaefer, Ronald P.; Egbokhare, Francis O.

doi:10.1349/ps1.1537-0852.a.443

Cited by 3 publications

(5 citation statements)

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“…Although we will primarily use Forker's approach, we will also exploit other similar approaches discussed in a thematic issue of Language Discovery from 2014. Apart from the paper written by Forker, that issue included contributions authored by Arka (2014), Creissels (2014), Haspelmath (2014), Schaefer and Egbokhare (2014), and Wichmann (2014: 1-2). In our view, the approach designed by Forker, enhanced by the above-mentioned typologically-driven and gradient proposals (cf.…”

Section: Theoretical Frameworkmentioning

confidence: 99%

“…For instance, arguments are expected to be marked for a grammatical case, whereas adjuncts are marked for a semantic case (Forker 2014: 31-32). Adjuncts can be introduced by overt relational predicates, whereas arguments cannot (Schaefer and Egbokhare 2014). As those diagnostics fail to be applicable to the Arusa language system, they are omitted in our list.…”

Section: D-5mentioning

confidence: 99%

“…As those diagnostics fail to be applicable to the Arusa language system, they are omitted in our list. For a review of other, more or less helpful diagnostics, consult Arka (2014), Creissels (2014), Forker (2014, Haspelmath (2014), and Schaefer and Egbokhare (2014). 8 Gradience and fuzziness characterize not only the argument-adjunct distinction in its totality, they are also symptomatic of each criterion and diagnostic individually.…”

Section: D-5mentioning

confidence: 99%

“…This study will be conducted within a canonical approach to the argument-adjunct distinction formulated by Forker (2014). This approach will additionally be complemented by similar methods proposed by Arka (2014), Schaefer and Egbokhare (2014), Creissels (2014), and Haspelmath (2014), and viewed as fully compatible with categorization methods used in cognitive linguistics (Janda 2015).…”

Section: Introductionmentioning

confidence: 99%

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Dative applicative elements in Arusa (Maa): A canonical approach to the argument-adjunct distinction

Andrason¹,

Karani

2019

SPILPLUS

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The present paper analyzes the degree of the argumenthood or adjuncthood of elements licensed by the dative applicative (DA) construction in Arusa within a canonical approach to the argument-adjunct distinction. After testing DA elements for the various criteria and diagnostics associated with the typologically-driven prototype of arguments and adjuncts, the authors conclude the following: in most cases, DA elements behave as canonical arguments and are therefore located close to the argumenthood pole of the argument-adjunct continuum.

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Section: Theoretical Frameworkmentioning

confidence: 99%

Section: D-5mentioning

confidence: 99%

Section: D-5mentioning

confidence: 99%

Section: Introductionmentioning

confidence: 99%

See 2 more Smart Citations

Dative applicative elements in Arusa (Maa): A canonical approach to the argument-adjunct distinction

Andrason¹,

Karani

2019

SPILPLUS

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“…The reason for the mismatch between the number of observed novae and the predicted rate is due to a number of issues, including extinction from interstellar dust, or the apparent location of the CV (i.e., eruptions occurring along a line of sight that passes close to the Sun). Indeed, studies performed by Schaefer (2014) showed a low efficiency of discovery: for novae with peak apparent magnitude of 6 the efficiency is 22 %, while for novae with V = 10 mag the efficiency drops to 9%. It is worth noting that about 800 nova candidates have been reported from M31 (Pietsch 2010), and nearly 400 from our own Galaxy, from which roughly 100 are expected to be RN masqueraded as CN (Pagnotta & Schaefer 2014).…”

Section: Classical Novaementioning

confidence: 99%

Three-dimensional SPH simulations of the interaction between the nova ejecta and the companion star

Figueira

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(English) Classical and Recurrent novae are thermonuclear explosions hosted by accreting white dwarfs in stellar binary systems. Material piles up on top of the white dwarf star under mildly degenerate conditions, driving a thermonuclear runaway. The energy released by the suite of nuclear processes operating at the envelope heats the material up to peak temperatures ranging from 100 to 400 MK. In these events, about 10^-3 - 10^-7 M¿, enriched in CNO and, sometimes, other intermediate-mass elements (e.g., Ne, Na, Mg, Al), are ejected into the interstellar medium. To date, most of the e¿orts undertaken in the modeling of classical nova outbursts have focused on the early stages of the explosion and ejection, ignoring the interaction of the ejecta, ¿rst with the accretion disk orbiting the white dwarf, and ultimately with the secondary star. In this thesis, a suite of three-dimensional, SPH (Smoothed Particle Hydrodynamics) simulations of the interaction between the nova ejecta, the accretion disk, and the stellar companion have been performed to ¿ll this gap, aimed at testing the in¿uence of the di¿erent parameters (e.g., mass and velocity of the ejecta, mass and geometry of the accretion disk, mass of the white dwarf, orbital period...) on the dynamical (and chemical) properties of di¿erent classical and recurrent nova systems. (Català) Les noves clàssiques i recurrents són explosions termonuclears produïdes per acreció de material sobre la superfície d'estrelles nanes blanques en sistemes estel·lars binaris. El material s'acumula en les capes externes de la nana blanca en condicions de degeneració parcial, donant lloc a una allau termonuclear. L'energia alliberada pels processos nuclears que operen a l'embolcall, escalfa el material fins a assolir temperatures màximes que oscil·len entre 100 i 400 MK. En aquests fenòmens estel·lars, aproximadament 10^-3 - 10^-7 masses solars, de material enriquit en elements del grup CNO i, a vegades, altres elements de massa intermèdia (com ara Ne, Na, Mg o Al), són expulsades al medi interestel·lar. Fins a la data, la majoria dels esforços realitzats en la modelització de les erupcions de noves clàssiques s'han centrat en les primeres etapes de l'explosió i ejecció, ignorant la interacció del material ejectat, primer amb el disc d'acreció que orbita al voltant de la nana blanca, i en última instància amb l'estrella secundària. En aquesta tesi, s'ha realitzat un conjunt de simulacions tridimensionals SPH (Smoothed-Particle Hydrodynamics) de la interacció entre el material ejectat, el disc d'acreció, i l'estrella secundària, amb la intenció d'omplir aquest buit en la caracterització de les explosions de noves. Bàsicament, hem analitzat la influència dels diferents paràmetres (per exemple, la massa i la velocitat del material ejectat, la massa i la geometria del disc d'acreció, la massa de la nana blanca, el període orbital...) en les propietats dinàmiques (i químiques) de diferents tipus de noves clàssiques i recurrents.

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Argument structure of emotive interjections: Evidence from Polish

Andrason

2022

Lingua

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Emai's Variable Coding of Adjuncts

Cited by 3 publications

References 2 publications

Dative applicative elements in Arusa (Maa): A canonical approach to the argument-adjunct distinction

Dative applicative elements in Arusa (Maa): A canonical approach to the argument-adjunct distinction

Three-dimensional SPH simulations of the interaction between the nova ejecta and the companion star

Argument structure of emotive interjections: Evidence from Polish

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