@article{Wendt2014,
  author    = {Wendt, Martin},
  title     = {Constraints on variations of m(p)/m(e) based on UVES observations of H-2},
  series = {Astronomische Nachrichten = Astronomical notes},
  volume    = {335},
  journal   = {Astronomische Nachrichten = Astronomical notes},
  number    = {1},
  publisher = {Wiley-VCH},
  address   = {Weinheim},
  issn      = {0004-6337},
  doi       = {10.1002/asna.201312008},
  pages     = {106 -- 112},
  year      = {2014},
  abstract  = {This article summarizes the latest results on the proton-to-electron mass ratio derived from H-2 observations at high redshift in the light of possible variations of fundamental physical constants. The focus lies on UVES observations of the past years as enormous progress was achieved since the first positive results on / were published. With the better understanding of systematics, dedicated observation runs, and numerous approaches to improve wavelength calibration accuracy, all current findings are in reasonable good agreement with no variation and provide an upper limit of / < 1 x 10(-5) for the redshift range of 2 < z < 3. ((},
  language  = {en}
}
@article{RichterFoxBenBekhtietal.2014,
  author    = {Richter, Philipp and Fox, Andrew J. and Ben Bekhti, Nadya and Murphy, M. T. and Bomans, Dominik J. and Frank, S.},
  title     = {High-resolution absorption spectroscopy of the circumgalactic medium of the Milky Way},
  series = {Astronomische Nachrichten = Astronomical notes},
  volume    = {335},
  journal   = {Astronomische Nachrichten = Astronomical notes},
  number    = {1},
  publisher = {Wiley-VCH},
  address   = {Weinheim},
  issn      = {0004-6337},
  doi       = {10.1002/asna.201312013},
  pages     = {92 -- 98},
  year      = {2014},
  language  = {en}
}
@article{BonifacioRahmaniWhitmoreetal.2014,
  author    = {Bonifacio, P. and Rahmani, H. and Whitmore, J. B. and Wendt, Martin and Centurion, Martin and Molaro, P. and Srianand, R. and Murphy, M. T. and Petitjean, P. and Agafonova, I. I. and Evans, T. M. and Levshakov, S. A. and Lopez, S. and Martins, C. J. A. P. and Reimers, D. and Vladilo, G.},
  title     = {Fundamental constants and high-resolution spectroscopy},
  series = {Astronomische Nachrichten = Astronomical notes},
  volume    = {335},
  journal   = {Astronomische Nachrichten = Astronomical notes},
  number    = {1},
  publisher = {Wiley-VCH},
  address   = {Weinheim},
  issn      = {0004-6337},
  doi       = {10.1002/asna.201312005},
  pages     = {83 -- 91},
  year      = {2014},
  language  = {en}
}
@article{FoxWakkerBargeretal.2014,
  author    = {Fox, Andrew J. and Wakker, Bart P. and Barger, Kathleen A. and Hernandez, Audra K. and Richter, Philipp and Lehner, Nicolas and Bland-Hawthorn, Joss and Charlton, Jane C. and Westmeier, Tobias and Thom, Christopher and Tumlinson, Jason and Misawa, Toru and Howk, J. Christopher and Haffner, L. Matthew and Ely, Justin and Rodriguez-Hidalgo, Paola and Kumari, Nimisha},
  title     = {The COS/UVES absorption survey of the magellanic stream. III. Ionization, total mass, and inflow rate onto the milky way},
  series = {The astrophysical journal : an international review of spectroscopy and astronomical physics},
  volume    = {787},
  journal   = {The astrophysical journal : an international review of spectroscopy and astronomical physics},
  number    = {2},
  publisher = {IOP Publ. Ltd.},
  address   = {Bristol},
  issn      = {0004-637X},
  doi       = {10.1088/0004-637X/787/2/147},
  pages     = {31},
  year      = {2014},
  abstract  = {Dynamic interactions between the two Magellanic Clouds have flung large quantities of gas into the halo of the Milky Way. The result is a spectacular arrangement of gaseous structures, including the Magellanic Stream, the Magellanic Bridge, and the Leading Arm (collectively referred to as the Magellanic System). In this third paper of a series studying the Magellanic gas in absorption, we analyze the gas ionization level using a sample of 69 Hubble Space Telescope/Cosmic Origins Spectrograph sightlines that pass through or within 30 degrees of the 21 cm emitting regions. We find that 81\% (56/69) of the sightlines show UV absorption at Magellanic velocities, indicating that the total cross-section of the Magellanic System is approximate to 11,000 deg(2), or around one-quarter of the entire sky. Using observations of the Si III/Si II ratio together with Cloudy photoionization modeling, we calculate the total gas mass (atomic plus ionized) of the Magellanic System to be approximate to 2.0 x 10(9) M-circle dot (d/55 kpc)(2), with the ionized gas contributing around three times as much mass as the atomic gas. This is larger than the current-day interstellar H I mass of both Magellanic Clouds combined, indicating that they have lost most of their initial gas mass. If the gas in the Magellanic System survives to reach the Galactic disk over its inflow time of similar to 0.5-1.0 Gyr, it will represent an average inflow rate of similar to 3.7-6.7 M-circle dot yr(-1), potentially raising the Galactic star formation rate. However, multiple signs of an evaporative interaction with the hot Galactic corona indicate that the Magellanic gas may not survive its journey to the disk fully intact and will instead add material to (and cool) the corona.},
  language  = {en}
}
@article{EvansMurphyWhitmoreetal.2014,
  author    = {Evans, T. M. and Murphy, M. T. and Whitmore, J. B. and Misawa, T. and Centurion, Martin and Lopez, S. and Martins, C. J. A. P. and Molaro, P. and Petitjean, P. and Rahmani, H. and Srianand, R. and Wendt, Martin},
  title     = {The UVES Large Program for testing fundamental physics - III. Constraints on the fine-structure constant from three telescopes},
  series = {Monthly notices of the Royal Astronomical Society},
  volume    = {445},
  journal   = {Monthly notices of the Royal Astronomical Society},
  number    = {1},
  publisher = {Oxford Univ. Press},
  address   = {Oxford},
  issn      = {0035-8711},
  doi       = {10.1093/mnras/stu1754},
  pages     = {128 -- 150},
  year      = {2014},
  language  = {en}
}