Zobrazeno 1 - 4
of 4
pro vyhledávání: '"L. M. Hogarth"'
Autor:
J. van de Sande, Julia J. Bryant, Matt S. Owers, Scott M. Croom, Brent Groves, Amélie Saintonge, L. M. Hogarth, Timothy A. Davis, Luca Cortese, Guido Roberts-Borsani, Joss Bland-Hawthorn, Edward N. Taylor, Sarah Brough, Thomas J. Fletcher, Angel R. Lopez-Sanchez, Samuel N. Richards, Jon Lawrence, Barbara Catinella, Nicholas Scott
We perform a joint-analysis of high spatial resolution molecular gas and star-formation rate (SFR) maps in main-sequence star-forming galaxies experiencing galactic-scale outflows of ionised gas. Our aim is to understand the mechanism that determines
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::259cd880cc3327096ddbc8adcb94c74e
http://arxiv.org/abs/2011.03566
http://arxiv.org/abs/2011.03566
Autor:
Ricardo Amorín, V. Firpo, Enrique Pérez-Montero, R. Chávez, A. Jaskot, Mónica V. Cardaci, Guillermo F. Hägele, L. M. Hogarth, José M. Vílchez
Publikováno v:
CONICET Digital (CONICET)
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Digital.CSIC. Repositorio Institucional del CSIC
instname
Consejo Nacional de Investigaciones Científicas y Técnicas
instacron:CONICET
Digital.CSIC. Repositorio Institucional del CSIC
instname
We investigate the ionized gas kinematics, physical properties, and chemical abundances of Sloan Digital Sky Survey J142947, a Green Pea galaxy at redshift z∼ 0.17 with strong, double-peak Ly α emission and indirect evidence of Lyman continuum (Ly
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b48fae1654cf9b7eb85af07a1903a37d
https://academic.oup.com/mnras/article-abstract/494/3/3541/5815438?redirectedFrom=fulltext
https://academic.oup.com/mnras/article-abstract/494/3/3541/5815438?redirectedFrom=fulltext
Publikováno v:
Monthly notices of the Royal Astronomical Society, 2019, Vol.490(4), pp.4715-4720 [Peer Reviewed Journal]
We revisit our mapping of the `Local Hole', a large underdensity in the local galaxy redshift distribution that extends out to redshift, $z\approx0.05$ and a potential source of outflows that may perturb the global expansion rate and thus help mitiga
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6049424b1569ad669b398cc6ee848882
http://arxiv.org/abs/1909.01878
http://arxiv.org/abs/1909.01878
Publikováno v:
Monthly notices of the Royal Astronomical Society : letters, 2019, Vol.484(1), pp.L64-L68 [Peer Reviewed Journal]
There is an $\approx9\pm2.5$\% tension between the value of Hubble's Constant, $H_0=67.4\pm0.5$km\,s$^{-1}$Mpc$^{-1}$, implied by the {\it Planck} microwave background power spectrum and that given by the distance scale of $H_0=73.4\pm1.7$km\,s$^{-1}
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9bbaf10fedea064823667e6b8bda2acc
http://dro.dur.ac.uk/28999/
http://dro.dur.ac.uk/28999/