TY  - JOUR
A1  - Georgi, Doreen
T1  - Patterns of movement reflexes as the result of the order of merge and agree
JF  - Linguistic Inquiry
N2  - In this article, I analyze patterns of reflexes of A-movement found within and across languages: reflexes may occur in all or none of the clauses of the dependency, in the clause where the dependency terminates, or solely in clauses where it does not terminate. I argue that the variation can best be captured by the variable timing of Agree and two subtypes of internal Merge (final vs. intermediate movement steps) triggered by a single head: early movement feeds Agree and gives rise to a reflex; late movement has the opposite effect. Since the subtypes of movement can apply at different points relative to Agree, reflexes may occur only in some clauses of the dependency.
KW  - movement reflexes
KW  - Agree
KW  - Merge
KW  - opacity
KW  - order of operations
KW  - optionality
Y1  - 2017
U6  - https://doi.org/10.1162/LING_a_00255
SN  - 0024-3892
SN  - 1530-9150
VL  - 48
IS  - 4
SP  - 585
EP  - 626
PB  - MIT Press
CY  - Cambridge
ER  - 
TY  - JOUR
A1  - Zacharias, Michael
A1  - Chen, Xuhui
A1  - Wagner, Stefan
T1  - Attenuation of TeV gamma-rays by the starlight photon field of the host galaxy
JF  - Monthly notices of the Royal Astronomical Society
N2  - The absorption of TeV gamma-ray photons produced in relativistic jets by surrounding soft photon fields is a long-standing problem of jet physics. In some cases, the most likely emission site close to the central black hole is ruled out because of the high opacity caused by strong optical and infrared photon sources, such as the broad-line region. Mostly neglected for jet modelling is the absorption of gamma-rays in the starlight photon field of the host galaxy. Analysing the absorption for arbitrary locations and observation angles of the gamma-ray emission site within the host galaxy, we find that the distance to the galaxy centre, the observation angle, and the distribution of starlight in the galaxy are crucial for the amount of absorption. We derive the absorption value for a sample of 20 TeV-detected blazars with a redshift z(r) < 0.2. The absorption value of the gamma-ray emission located in the galaxy centre may be as high as 20 per cent, with an average value of 6 per cent. This is important in order to determine the intrinsic blazar parameters. We see no significant trends in our sample between the degree of absorption and host properties, such as starlight emissivity, galactic size, half-light radius, and redshift. While the uncertainty of the spectral properties of the extragalactic background light exceeds the effect of absorption by stellar light from the host galaxy in distant objects, the latter is a dominant effect in nearby sources. It may also be revealed in a differential comparison of sources with similar redshifts.
KW  - opacity
KW  - radiation mechanisms: non-thermal
KW  - galaxies: active
KW  - gamma-rays: galaxies
Y1  - 2016
U6  - https://doi.org/10.1093/mnras/stw3032
SN  - 0035-8711
SN  - 1365-2966
VL  - 465
IS  - 3
SP  - 3767
EP  - 3774
PB  - Oxford Univ. Press
CY  - Oxford
ER  -