Search Publications

Sizes, colour gradients and resolved stellar mass distributions for the massive cluster galaxies in XMMUJ2235-2557 at z = 1.39
DOI: 10.1093/mnras/stw502 Bibcode: 2016MNRAS.458.3181C

Bender, Ralf; Mendel, J. Trevor; Cappellari, Michele +13 more

We analyse the sizes, colour gradients and resolved stellar mass distributions for 36 massive and passive galaxies in the cluster XMMUJ2235-2557 at z = 1.39 using optical and near-infrared Hubble Space Telescope (HST) imaging. We derive light-weighted Sérsic fits in five HST bands (I775, z850, Y105, J125

2016 Monthly Notices of the Royal Astronomical Society
eHST 48
The outburst decay of the low magnetic field magnetar SWIFT J1822.3-1606: phase-resolved analysis and evidence for a variable cyclotron feature
DOI: 10.1093/mnras/stv2490 Bibcode: 2016MNRAS.456.4145R

Mereghetti, Sandro; Esposito, Paolo; Turolla, Roberto +12 more

We study the timing and spectral properties of the low-magnetic field, transient magnetar SWIFT J1822.3-1606 as it approached quiescence. We coherently phase-connect the observations over a time-span of ∼500 d since the discovery of SWIFT J1822.3-1606 following the Swift-Burst Alert Telescope (BAT) trigger on 2011 July 14, and carried out a detail…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 48
The Hubble Space Telescope UV Legacy Survey of Galactic Globular Clusters. VII. Implications from the Nearly Universal Nature of Horizontal Branch Discontinuities
DOI: 10.3847/0004-637X/822/1/44 Bibcode: 2016ApJ...822...44B

Dalessandro, E.; Salaris, M.; Anderson, J. +14 more

The UV-initiative Hubble Space Telescope Treasury survey of Galactic globular clusters provides a new window into the phenomena that shape the morphological features of the horizontal branch (HB). Using this large and homogeneous catalog of UV and blue photometry, we demonstrate that the HB exhibits discontinuities that are remarkably consistent i…

2016 The Astrophysical Journal
eHST 48
High-velocity extended molecular outflow in the star-formation dominated luminous infrared galaxy ESO 320-G030
DOI: 10.1051/0004-6361/201628875 Bibcode: 2016A&A...594A..81P

Colina, L.; Villar-Martín, M.; Planesas, P. +9 more

We analyze new high spatial resolution (~60 pc) ALMA CO(2-1) observations of the isolated luminous infrared galaxy ESO 320-G030 (d = 48 Mpc) in combination with ancillary Hubble Space Telescope optical and near infrared (IR) imaging, as well as VLT/SINFONI near-IR integral field spectroscopy. We detect a high-velocity (~450 km s-1) spat…

2016 Astronomy and Astrophysics
Herschel eHST 47
Extinction law in the range 0.4-4.8 µm and the 8620 Å DIB towards the stellar cluster Westerlund 1
DOI: 10.1093/mnras/stw2122 Bibcode: 2016MNRAS.463.2653D

Rubinho, M. S.; Almeida, L. A.; Damineli, A. +4 more

The young stellar cluster Westerlund 1 (Wd 1: l = 339.6°, b = -0.4°) is one of the most massive in the local Universe, but accurate parameters are pending on better determination of its extinction and distance. Based on our photometry and data collected from other sources, we have derived a reddening law for the cluster line-of-sight representativ…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 47
Sulphur molecules in the circumstellar envelopes of M-type AGB stars
DOI: 10.1051/0004-6361/201527943 Bibcode: 2016A&A...588A.119D

Olofsson, H.; Justtanont, K.; Black, J. H. +2 more


Aims: The sulphur compounds SO and SO2 have not been widely studied in the circumstellar envelopes of asymptotic giant branch (AGB) stars. By presenting and modelling a large number of SO and SO2 lines in the low mass-loss rate M-type AGB star R Dor, and modelling the available lines of those molecules in a further four …

2016 Astronomy and Astrophysics
Herschel 47
Mass-loading, pile-up, and mirror-mode waves at comet 67P/Churyumov-Gerasimenko
DOI: 10.5194/angeo-34-1-2016 Bibcode: 2016AnGeo..34....1V

Altwegg, K.; Glassmeier, K. -H.; Nilsson, H. +23 more

The data from all Rosetta plasma consortium instruments and from the ROSINA COPS instrument are used to study the interaction of the solar wind with the outgassing cometary nucleus of 67P/Churyumov-Gerasimenko. During 6 and 7 June 2015, the interaction was first dominated by an increase in the solar wind dynamic pressure, caused by a higher solar …

2016 Annales Geophysicae
Rosetta 47
SPT-GMOS: A Gemini/GMOS-South Spectroscopic Survey of Galaxy Clusters in the SPT-SZ Survey
DOI: 10.3847/0067-0049/227/1/3 Bibcode: 2016ApJS..227....3B

Bayliss, M. B.; Gladders, M. D.; Schrabback, T. +75 more

We present the results of SPT-GMOS, a spectroscopic survey with the Gemini Multi-Object Spectrograph (GMOS) on Gemini South. The targets of SPT-GMOS are galaxy clusters identified in the SPT-SZ survey, a millimeter-wave survey of 2500 deg2 of the southern sky using the South Pole Telescope (SPT). Multi-object spectroscopic observations …

2016 The Astrophysical Journal Supplement Series
eHST 47
Surface Albedo and Spectral Variability of Ceres
DOI: 10.3847/2041-8205/817/2/L22 Bibcode: 2016ApJ...817L..22L

Nathues, Andreas; Schröder, Stefan E.; Russell, Christopher T. +21 more

Previous observations suggested that Ceres has active, but possibly sporadic, water outgassing as well as possibly varying spectral characteristics over a timescale of months. We used all available data of Ceres collected in the past three decades from the ground and the Hubble Space Telescope, as well as the newly acquired images by the Dawn  Fra…

2016 The Astrophysical Journal
eHST 47
Close stellar conjunctions of α Centauri A and B until 2050 . An mK = 7.8 star may enter the Einstein ring of α Cen A in 2028
DOI: 10.1051/0004-6361/201629201 Bibcode: 2016A&A...594A.107K

Kervella, P.; Mignard, F.; Thévenin, F. +1 more

The rapid proper motion of the α Cen pair (≈3.7 arcsec yr-1) and its location close to the galactic plane on a rich stellar background combine constructively to make them excellent candidates for close stellar conjunctions with more distant stars. Adding new differential astrometry to archival data, we have refined the orbital parameter…

2016 Astronomy and Astrophysics
XMM-Newton 47