Zobrazeno 1 - 10
of 37
pro vyhledávání: '"N Quirk"'
Autor:
CJ Peniche Silva, SA Müller, N Quirk, RE De la Vega, MJ Coenen, CH Evans, ER Balmayor, M van Griensven
Publikováno v:
European Cells & Materials, Vol 44, Pp 43-55 (2022)
The interphase between tendon and bone consists of a highly specialised tissue called enthesis. Typically, the enthesis is described as a succession of four different zones: tendon, non-mineralised fibrocartilage, mineralised fibrocartilage and bone.
Externí odkaz:
https://doaj.org/article/2da97e09d94d4b1fad71d50c4618a74a
Autor:
CV Nagelli, A Hooke, N Quirk, CL De Padilla, TE Hewett, M van Griensven, M Coenen, L Berglund, CH Evans, SA Müller
Publikováno v:
European Cells & Materials, Vol 43, Pp 153-161 (2022)
The Achilles tendon is the strongest tendon in the human body but its mechanical behaviour during failure has been little studied and the basis of its high tensile strength has not been elucidated in detail. In the present study, healthy, human, Achi
Externí odkaz:
https://doaj.org/article/c02cec0f7dbc456bbfe9d2af8b6eb653
Autor:
L. R. Cullinane, Karoline M. Gilbert, Puragra Guhathakurta, A. C. N. Quirk, Ivanna Escala, Adam Smercina, Benjamin F. Williams, Erik Tollerud, Jessamine Qu, Kaela McConnell
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 2, p 157 (2023)
The dwarf galaxy Triangulum (M33) presents an interesting testbed for studying stellar halo formation: it is sufficiently massive so as to have likely accreted smaller satellites, but also lies within the regime where feedback and other “in situ”
Externí odkaz:
https://doaj.org/article/b0bf4192709f4604a3a67629ec85ed61
Autor:
Adam Smercina, Julianne J. Dalcanton, Benjamin F. Williams, Meredith J. Durbin, Margaret Lazzarini, Eric F. Bell, Yumi Choi, Andrew Dolphin, Karoline Gilbert, Puragra Guhathakurta, Eric W. Koch, Amanda C. N. Quirk, Hans-Walter Rix, Erik Rosolowsky, Anil Seth, Evan Skillman, Daniel R. Weisz
Publikováno v:
The Astrophysical Journal, Vol 957, Iss 1, p 3 (2023)
We present a detailed analysis of the structure of the Local Group flocculent spiral galaxy M33, as measured using the Panchromatic Hubble Andromeda Treasury Triangulum Extended Region (PHATTER) survey. Leveraging the multiwavelength coverage of PHAT
Externí odkaz:
https://doaj.org/article/996ac5beb87c49be83b18a04c3a5bf59
Autor:
Ivanna Escala, Amanda C. N. Quirk, Puragra Guhathakurta, Karoline M. Gilbert, J. Leigh Wojno, Lara Cullinane, Benjamin F. Williams, Julianne Dalcanton
Publikováno v:
The Astronomical Journal, Vol 165, Iss 2, p 75 (2023)
Stellar kinematics and metallicity are key to exploring formation scenarios for galactic disks and halos. In this work, we characterized the relationship between kinematics and photometric metallicity along the line of sight to M31's disk. We combine
Externí odkaz:
https://doaj.org/article/8796b2e8619f43fb9b526996c105b0cf
Autor:
Ivanna Escala, Amanda C. N. Quirk, Puragra Guhathakurta, Karoline M. Gilbert, J. Leigh Wojno, Lara Cullinane, Benjamin F. Williams, Julianne Dalcanton
Stellar kinematics and metallicity are key to exploring formation scenarios for galactic disks and halos. In this work, we characterized the relationship between kinematics and photometric metallicity along the line-of-sight to M31's disk. We combine
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d993482eda73bd2d165f188a89985e2
http://arxiv.org/abs/2209.07962
http://arxiv.org/abs/2209.07962
Autor:
Ekta Patel, Amanda C. N. Quirk
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 497:2870-2882
We analyze the kinematics as a function of stellar age for Andromeda (M31) mass analogs from the IllustrisTNG cosmological simulation. We divide the star particles into four age groups: less than 1 Gyr, 1 to 5 Gyr, 5 to 10 Gyr, and greater 10 Gyr, an
The Triangulum Extended (TREX) Survey: The Stellar Disk Dynamics of M33 as a Function of Stellar Age
Autor:
Amanda C. N. Quirk, Puragra Guhathakurta, Karoline M. Gilbert, Laurent Chemin, Julianne J. Dalcanton, Benjamin F. Williams, Anil Seth, Ekta Patel, Justin T. Fung, Pujita Tangirala, Ibrahim Yusufali
Triangulum, M33, is a low mass, relatively undisturbed spiral galaxy that offers a new regime in which to test models of dynamical heating. In spite of its proximity, the dynamical heating history of M33 has not yet been well constrained. In this wor
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::feea5be27c3fcb72a33969a79cc08ffe
Autor:
Karoline M. Gilbert, Amanda C. N. Quirk, Puragra Guhathakurta, Erik Tollerud, Jennifer Wojno, Julianne J. Dalcanton, Meredith J. Durbin, Anil Seth, Benjamin F. Williams, Justin T. Fung, Pujita Tangirala, Ibrahim Yusufali
We present initial results from a large spectroscopic survey of stars throughout M33's stellar disk. We analyze a sample of 1667 red giant branch (RGB) stars extending to projected distances of $\sim 11$ kpc from M33's center ($\sim 18$ kpc, or $\sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8d7d9e66db2d7de373b7814720e801cb
http://arxiv.org/abs/2110.15773
http://arxiv.org/abs/2110.15773
Autor:
Karoline M. Gilbert, Amanda C. N. Quirk, Puragra Guhathakurta, Erik Tollerud, Jennifer Wojno, Julianne J. Dalcanton, Meredith J. Durbin, Anil Seth, Benjamin F. Williams, Justin T. Fung, Pujita Tangirala, Ibrahim Yusufali
Publikováno v:
The Astrophysical Journal. 931:169