@misc{swinbank2017angular,
  abstract = {We present a MUSE and KMOS dynamical study 405 star-forming galaxies at
redshift z=0.28-1.65 (median redshift z=0.84). Our sample are representative of
star-forming, main-sequence galaxies, with star-formation rates of
SFR=0.1-30Mo/yr and stellar masses M=10^8-10^11Mo. For 49+/-4% of our sample,
the dynamics suggest rotational support, 24+/-3% are unresolved systems and
5+/-2% appear to be early-stage major mergers with components on 8-30kpc
scales. The remaining 22+/-5% appear to be dynamically complex, irregular (or
face-on systems). For galaxies whose dynamics suggest rotational support, we
derive inclination corrected rotational velocities and show these systems lie
on a similar scaling between stellar mass and specific angular momentum as
local spirals with j*=J/M*\propto M^(2/3) but with a redshift evolution that
scales as j*\propto M^{2/3}(1+z)^(-1). We identify a correlation between
specific angular momentum and disk stability such that galaxies with the
highest specific angular momentum, log(j*/M^(2/3))>2.5, are the most stable,
with Toomre Q=1.10+/-0.18, compared to Q=0.53+/-0.22 for galaxies with
log(j*/M^(2/3))<2.5. At a fixed mass, the HST morphologies of galaxies with the
highest specific angular momentum resemble spiral galaxies, whilst those with
low specific angular momentum are morphologically complex and dominated by
several bright star-forming regions. This suggests that angular momentum plays
a major role in defining the stability of gas disks: at z~1, massive galaxies
that have disks with low specific angular momentum, appear to be globally
unstable, clumpy and turbulent systems. In contrast, galaxies with high
specific angular have evolved in to stable disks with spiral structures.},
  added-at = {2017-01-27T11:07:05.000+0100},
  author = {Swinbank, Mark and Harrison, Chris and Trayford, James and Schaller, Matthieu and Smail, Ian and Schaye, Joop and Theuns, Tom and Smit, Renske and Alexander, David and Bacon, Roland and Bower, Richard and Contini, Thierry and Crain, Rob and de Breuck, Carlos and Decarli, Roberto and Epinat, Benoit and Fumagalli, Michele and Furlong, Michelle and Galametz, Audrey and Johnson, Helen and Lagos, Claudia and Richard, Johan and Vernet, Joel and Sharples, Ray and Sobral, David and Stott, John},
  biburl = {https://www.bibsonomy.org/bibtex/2830b09bab83c479a5046608c1eac6a15/miki},
  description = {[1701.07448] Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7},
  interhash = {6b7278b70d4f64f9c3817afba9eeb3f5},
  intrahash = {830b09bab83c479a5046608c1eac6a15},
  keywords = {momentum angular galaxies z~1},
  note = {cite arxiv:1701.07448Comment: MNRAS in press. 21 pages; 12 figures. The full pdf, which includes an  additional 32 pages of supplementary figures and data tables are available  from http://astro.dur.ac.uk/~ams/MUSEcubes/},
  timestamp = {2017-01-27T11:07:05.000+0100},
  title = {Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and
  KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7},
  url = {http://arxiv.org/abs/1701.07448},
  year = 2017
}

{"_id":"hGFiPFc2siAQsBdWx","bibbaseid":"swinbank-harrison-trayford-schaller-smail-schaye-theuns-smit-etal-angularmomentumevolutionofgalaxiesoverthepast10gyramuseandkmosdynamicalsurveyof400starforminggalaxiesfromz0317-2017","author_short":["Swinbank, M.","Harrison, C.","Trayford, J.","Schaller, M.","Smail, I.","Schaye, J.","Theuns, T.","Smit, R.","Alexander, D.","Bacon, R.","Bower, R.","Contini, T.","Crain, R.","de Breuck, C.","Decarli, R.","Epinat, B.","Fumagalli, M.","Furlong, M.","Galametz, A.","Johnson, H.","Lagos, C.","Richard, J.","Vernet, J.","Sharples, R.","Sobral, D.","Stott, J."],"bibdata":{"bibtype":"misc","type":"misc","abstract":"We present a MUSE and KMOS dynamical study 405 star-forming galaxies at redshift z=0.28-1.65 (median redshift z=0.84). Our sample are representative of star-forming, main-sequence galaxies, with star-formation rates of SFR=0.1-30Mo/yr and stellar masses M=10^8-10^11Mo. For 49+/-4% of our sample, the dynamics suggest rotational support, 24+/-3% are unresolved systems and 5+/-2% appear to be early-stage major mergers with components on 8-30kpc scales. The remaining 22+/-5% appear to be dynamically complex, irregular (or face-on systems). For galaxies whose dynamics suggest rotational support, we derive inclination corrected rotational velocities and show these systems lie on a similar scaling between stellar mass and specific angular momentum as local spirals with j*=J/M*∝ M^(2/3) but with a redshift evolution that scales as j*∝ M^2/3(1+z)^(-1). We identify a correlation between specific angular momentum and disk stability such that galaxies with the highest specific angular momentum, log(j*/M^(2/3))>2.5, are the most stable, with Toomre Q=1.10+/-0.18, compared to Q=0.53+/-0.22 for galaxies with log(j*/M^(2/3))<2.5. At a fixed mass, the HST morphologies of galaxies with the highest specific angular momentum resemble spiral galaxies, whilst those with low specific angular momentum are morphologically complex and dominated by several bright star-forming regions. This suggests that angular momentum plays a major role in defining the stability of gas disks: at z 1, massive galaxies that have disks with low specific angular momentum, appear to be globally unstable, clumpy and turbulent systems. In contrast, galaxies with high specific angular have evolved in to stable disks with spiral structures.","added-at":"2017-01-27T11:07:05.000+0100","author":[{"propositions":[],"lastnames":["Swinbank"],"firstnames":["Mark"],"suffixes":[]},{"propositions":[],"lastnames":["Harrison"],"firstnames":["Chris"],"suffixes":[]},{"propositions":[],"lastnames":["Trayford"],"firstnames":["James"],"suffixes":[]},{"propositions":[],"lastnames":["Schaller"],"firstnames":["Matthieu"],"suffixes":[]},{"propositions":[],"lastnames":["Smail"],"firstnames":["Ian"],"suffixes":[]},{"propositions":[],"lastnames":["Schaye"],"firstnames":["Joop"],"suffixes":[]},{"propositions":[],"lastnames":["Theuns"],"firstnames":["Tom"],"suffixes":[]},{"propositions":[],"lastnames":["Smit"],"firstnames":["Renske"],"suffixes":[]},{"propositions":[],"lastnames":["Alexander"],"firstnames":["David"],"suffixes":[]},{"propositions":[],"lastnames":["Bacon"],"firstnames":["Roland"],"suffixes":[]},{"propositions":[],"lastnames":["Bower"],"firstnames":["Richard"],"suffixes":[]},{"propositions":[],"lastnames":["Contini"],"firstnames":["Thierry"],"suffixes":[]},{"propositions":[],"lastnames":["Crain"],"firstnames":["Rob"],"suffixes":[]},{"propositions":["de"],"lastnames":["Breuck"],"firstnames":["Carlos"],"suffixes":[]},{"propositions":[],"lastnames":["Decarli"],"firstnames":["Roberto"],"suffixes":[]},{"propositions":[],"lastnames":["Epinat"],"firstnames":["Benoit"],"suffixes":[]},{"propositions":[],"lastnames":["Fumagalli"],"firstnames":["Michele"],"suffixes":[]},{"propositions":[],"lastnames":["Furlong"],"firstnames":["Michelle"],"suffixes":[]},{"propositions":[],"lastnames":["Galametz"],"firstnames":["Audrey"],"suffixes":[]},{"propositions":[],"lastnames":["Johnson"],"firstnames":["Helen"],"suffixes":[]},{"propositions":[],"lastnames":["Lagos"],"firstnames":["Claudia"],"suffixes":[]},{"propositions":[],"lastnames":["Richard"],"firstnames":["Johan"],"suffixes":[]},{"propositions":[],"lastnames":["Vernet"],"firstnames":["Joel"],"suffixes":[]},{"propositions":[],"lastnames":["Sharples"],"firstnames":["Ray"],"suffixes":[]},{"propositions":[],"lastnames":["Sobral"],"firstnames":["David"],"suffixes":[]},{"propositions":[],"lastnames":["Stott"],"firstnames":["John"],"suffixes":[]}],"biburl":"https://www.bibsonomy.org/bibtex/2830b09bab83c479a5046608c1eac6a15/miki","description":"[1701.07448] Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7","interhash":"6b7278b70d4f64f9c3817afba9eeb3f5","intrahash":"830b09bab83c479a5046608c1eac6a15","keywords":"momentum angular galaxies z 1","note":"cite arxiv:1701.07448Comment: MNRAS in press. 21 pages; 12 figures. The full pdf, which includes an additional 32 pages of supplementary figures and data tables are available from http://astro.dur.ac.uk/ ams/MUSEcubes/","timestamp":"2017-01-27T11:07:05.000+0100","title":"Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7","url":"http://arxiv.org/abs/1701.07448","year":"2017","bibtex":"@misc{swinbank2017angular,\n abstract = {We present a MUSE and KMOS dynamical study 405 star-forming galaxies at\r\nredshift z=0.28-1.65 (median redshift z=0.84). Our sample are representative of\r\nstar-forming, main-sequence galaxies, with star-formation rates of\r\nSFR=0.1-30Mo/yr and stellar masses M=10^8-10^11Mo. For 49+/-4% of our sample,\r\nthe dynamics suggest rotational support, 24+/-3% are unresolved systems and\r\n5+/-2% appear to be early-stage major mergers with components on 8-30kpc\r\nscales. The remaining 22+/-5% appear to be dynamically complex, irregular (or\r\nface-on systems). For galaxies whose dynamics suggest rotational support, we\r\nderive inclination corrected rotational velocities and show these systems lie\r\non a similar scaling between stellar mass and specific angular momentum as\r\nlocal spirals with j*=J/M*\\propto M^(2/3) but with a redshift evolution that\r\nscales as j*\\propto M^{2/3}(1+z)^(-1). We identify a correlation between\r\nspecific angular momentum and disk stability such that galaxies with the\r\nhighest specific angular momentum, log(j*/M^(2/3))>2.5, are the most stable,\r\nwith Toomre Q=1.10+/-0.18, compared to Q=0.53+/-0.22 for galaxies with\r\nlog(j*/M^(2/3))<2.5. At a fixed mass, the HST morphologies of galaxies with the\r\nhighest specific angular momentum resemble spiral galaxies, whilst those with\r\nlow specific angular momentum are morphologically complex and dominated by\r\nseveral bright star-forming regions. This suggests that angular momentum plays\r\na major role in defining the stability of gas disks: at z~1, massive galaxies\r\nthat have disks with low specific angular momentum, appear to be globally\r\nunstable, clumpy and turbulent systems. In contrast, galaxies with high\r\nspecific angular have evolved in to stable disks with spiral structures.},\n added-at = {2017-01-27T11:07:05.000+0100},\n author = {Swinbank, Mark and Harrison, Chris and Trayford, James and Schaller, Matthieu and Smail, Ian and Schaye, Joop and Theuns, Tom and Smit, Renske and Alexander, David and Bacon, Roland and Bower, Richard and Contini, Thierry and Crain, Rob and de Breuck, Carlos and Decarli, Roberto and Epinat, Benoit and Fumagalli, Michele and Furlong, Michelle and Galametz, Audrey and Johnson, Helen and Lagos, Claudia and Richard, Johan and Vernet, Joel and Sharples, Ray and Sobral, David and Stott, John},\n biburl = {https://www.bibsonomy.org/bibtex/2830b09bab83c479a5046608c1eac6a15/miki},\n description = {[1701.07448] Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7},\n interhash = {6b7278b70d4f64f9c3817afba9eeb3f5},\n intrahash = {830b09bab83c479a5046608c1eac6a15},\n keywords = {momentum angular galaxies z~1},\n note = {cite arxiv:1701.07448Comment: MNRAS in press. 21 pages; 12 figures. The full pdf, which includes an additional 32 pages of supplementary figures and data tables are available from http://astro.dur.ac.uk/~ams/MUSEcubes/},\n timestamp = {2017-01-27T11:07:05.000+0100},\n title = {Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and\r\n KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7},\n url = {http://arxiv.org/abs/1701.07448},\n year = 2017\n}\n\n","author_short":["Swinbank, M.","Harrison, C.","Trayford, J.","Schaller, M.","Smail, I.","Schaye, J.","Theuns, T.","Smit, R.","Alexander, D.","Bacon, R.","Bower, R.","Contini, T.","Crain, R.","de Breuck, C.","Decarli, R.","Epinat, B.","Fumagalli, M.","Furlong, M.","Galametz, A.","Johnson, H.","Lagos, C.","Richard, J.","Vernet, J.","Sharples, R.","Sobral, D.","Stott, J."],"key":"swinbank2017angular","id":"swinbank2017angular","bibbaseid":"swinbank-harrison-trayford-schaller-smail-schaye-theuns-smit-etal-angularmomentumevolutionofgalaxiesoverthepast10gyramuseandkmosdynamicalsurveyof400starforminggalaxiesfromz0317-2017","role":"author","urls":{"Paper":"http://arxiv.org/abs/1701.07448"},"keyword":["momentum angular galaxies z 1"],"metadata":{"authorlinks":{}},"downloads":0,"html":""},"bibtype":"misc","biburl":"http://www.bibsonomy.org/bib/author/Bower?items=1000","dataSources":["njK9TZffut9425riF"],"keywords":["momentum angular galaxies z 1"],"search_terms":["angular","momentum","evolution","galaxies","over","past","gyr","muse","kmos","dynamical","survey","400","star","forming","galaxies","swinbank","harrison","trayford","schaller","smail","schaye","theuns","smit","alexander","bacon","bower","contini","crain","de breuck","decarli","epinat","fumagalli","furlong","galametz","johnson","lagos","richard","vernet","sharples","sobral","stott"],"title":"Angular momentum evolution of galaxies over the past 10-Gyr: A MUSE and KMOS dynamical survey of 400 star-forming galaxies from z=0.3-1.7","year":2017}