Zobrazeno 1 - 10
of 30
pro vyhledávání: '"Jillian M Scudder"'
Autor:
Hsi-An Pan, Lihwai Lin, Sara L. Ellison, Mallory D. Thorp, Sebastián F. Sánchez, Asa F. L. Bluck, Francesco Belfiore, Joanna M. Piotrowska, Jillian M. Scudder, William M. Baker
Publikováno v:
The Astrophysical Journal, Vol 964, Iss 2, p 120 (2024)
Star formation quenching is one of the key processes that shape the evolution of galaxies. In this study, we investigate the changes in molecular gas and star formation properties as galaxies transit from the star-forming main sequence to the passive
Externí odkaz:
https://doaj.org/article/beb4ec73ab4b45ce9d0e1bec9d01a993
Autor:
Mallory D Thorp, Sara L Ellison, Hsi-An Pan, Lihwai Lin, David R Patton, Asa F L Bluck, Dan Walters, Jillian M Scudder
Galaxy mergers are known to trigger both extended and central star formation. However, what remains to be understood is whether this triggered star formation is facilitated by enhanced star formation efficiencies, or an abundance of molecular gas fue
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::24b24afe87daeafa762e7fd723324790
http://arxiv.org/abs/2208.06426
http://arxiv.org/abs/2208.06426
Autor:
William Matzko, Shobita Satyapal, Sara L Ellison, Remington O Sexton, Nathan J Secrest, Gabriela Canalizo, Laura Blecha, David R Patton, Jillian M Scudder
Powerful outflows are thought to play a critical role in galaxy evolution and black hole growth. We present the first large-scale systematic study of ionised outflows in paired galaxies and post-mergers compared to a robust control sample of isolated
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f52aa3405f169d2d0b8c0108878259b1
We present polynomial conversions between each of 11 different strong line gas-phase metallicity calibrations, each based on $\sim$ 1.1 million star-forming spaxels in the public Sloan Digital Sky Survey (SDSS) Data Release 15 (DR15) Mapping Nearby G
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83314a2204b5c3772d356274084c7d6c
http://arxiv.org/abs/2108.04934
http://arxiv.org/abs/2108.04934
Strong line metallicity calibrations are widely used to determine the gas phase metallicities of individual HII regions and entire galaxies. Over a decade ago, based on the Sloan Digital Sky Survey Data Release 4 (SDSS DR4), Kewley \& Ellison publish
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9a9179385ec8a109cad19d510fa2da72
http://arxiv.org/abs/2102.07058
http://arxiv.org/abs/2102.07058
Autor:
Lihwai Lin, Mallory D. Thorp, Sara L. Ellison, Hsi-An Pan, Asa F. L. Bluck, Sebastián F. Sánchez, Jillian M. Scudder, Roberto Maiolino
Using a sample of ~15,000 kpc-scale star-forming spaxels in 28 galaxies drawn from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we investigate the galaxy-to-galaxy variation of the `resolved' Schmidt-Kennicutt relation (rSK; Sigma_
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d40bb713e3e15ec02b24282620e5286
https://www.repository.cam.ac.uk/handle/1810/315113
https://www.repository.cam.ac.uk/handle/1810/315113
Autor:
Mallory D. Thorp, Lihwai Lin, Mark Sargent, Asa F. L. Bluck, Hsi-An Pan, Sara L. Ellison, Sebastián F. Sánchez, Jillian M. Scudder
Starburst galaxies have elevated star formation rates (SFRs) for their stellar mass. In Ellison et al. (2018) we used integral field unit (IFU) maps of star formation rate surface density (Sigma_SFR) and stellar mass surface density (Sigma_*) to show
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::accde34fc674d16bb630ba3b9f972a15
http://sro.sussex.ac.uk/id/eprint/90291/4/__smbhome.uscs.susx.ac.uk_tjk30_Documents_untitled.pdf
http://sro.sussex.ac.uk/id/eprint/90291/4/__smbhome.uscs.susx.ac.uk_tjk30_Documents_untitled.pdf
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2018, Vol.480(3), pp.4124-4137 [Peer Reviewed Journal]
Monthly Notices of the Royal Astronomical Society, 480(3), 4124-4137. Oxford University Press
Monthly Notices of the Royal Astronomical Society, 480(3), 4124-4137. Oxford University Press
In this paper, we investigate the physical associations between blended far-infrared (FIR)-emitting galaxies, in order to identify the level of line-of-sight projection contamination in the single-dish Herschel data. Building on previous work, and as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05b1edfad93308fe6a28049d38f82b8a
https://doi.org/10.1093/mnras/sty2009
https://doi.org/10.1093/mnras/sty2009
Autor:
Trevor Mendel, Sara L. Ellison, Mark Sargent, Kristen Coppin, Giulio Violino, Jillian M. Scudder, Amélie Saintonge
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 476:2591-2604
We investigate the connection between star formation and molecular gas properties in galaxy mergers at low redshift (z$\leq$0.06). The study we present is based on IRAM 30-m CO(1-0) observations of 11 galaxies with a close companion selected from the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f000aa8fb7d98897474652496383efcd
https://doi.org/10.1093/mnras/sty345
https://doi.org/10.1093/mnras/sty345
Autor:
Sara L. Ellison, Asa F. L. Bluck, Lihwai Lin, Jillian M. Scudder, Hsi-An Pan, Mark Sargent, Hossen Teimoorinia, Mallory D. Thorp, Sebastián F. Sánchez
Using a sample of 11,478 spaxels in 34 galaxies with molecular gas, star formation and stellar maps taken from the ALMA-MaNGA QUEnching and STar formation (ALMaQUEST) survey, we investigate the parameters that correlate with variations in star format
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a2f61852da0e30ddd408ed45b32d5a5f
http://arxiv.org/abs/1911.11887
http://arxiv.org/abs/1911.11887