Search Publications

Formation of bi-lobed shapes by sub-catastrophic collisions. A late origin of comet 67P's structure
DOI: 10.1051/0004-6361/201628964 Bibcode: 2017A&A...597A..62J

Benz, W.; Jutzi, M.

Context. The origin of the particular shape of comet 67P/Churyumov-Gerasimenko (67P) is a topic of active research. How and when it acquired its peculiar characteristics has distinct implications on the origin of the solar system and its dynamics.
Aims: We investigate how shapes such as that of comet 67P can result from a new type of low-ener…

2017 Astronomy and Astrophysics
Rosetta 72
Do galaxies that leak ionizing photons have extreme outflows?
DOI: 10.1051/0004-6361/201730610 Bibcode: 2017A&A...605A..67C

Chisholm, J.; Schaerer, D.; Thuan, T. X. +5 more

Context. To reionize the early universe, high-energy photons must escape the galaxies that produce them. How these photons escape is debated because too many ionizing photons are absorbed even at small H I column densities. It has been suggested that stellar feedback drives galactic outflows out of star-forming regions, creating low density channe…

2017 Astronomy and Astrophysics
eHST 72
The Complete Local Volume Groups Sample - I. Sample selection and X-ray properties of the high-richness subsample
DOI: 10.1093/mnras/stx2078 Bibcode: 2017MNRAS.472.1482O

Babul, Arif; Raychaudhury, Somak; Ponman, Trevor J. +7 more

We present the Complete Local-Volume Groups Sample (CLoGS), a statistically complete optically selected sample of 53 groups within 80 Mpc. Our goal is to combine X-ray, radio and optical data to investigate the relationship between member galaxies, their active nuclei and the hot intra-group medium (IGM). We describe sample selection, define a 26-…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 72
Interstellar Pickup Ion Observations to 38 au
DOI: 10.3847/1538-4365/aa91d2 Bibcode: 2017ApJS..233....8M

McComas, D. J.; Schwadron, N. A.; Szalay, J. R. +9 more

We provide the first direct observations of interstellar H+ and He+ pickup ions in the solar wind from 22 to 38 au. We use the Vasyliunas and Siscoe model functional form to quantify the pickup ion distributions, and while the fit parameters generally lie outside their physically expected ranges, this form allows fits that qu…

2017 The Astrophysical Journal Supplement Series
Ulysses 72
BANYAN. IX. The Initial Mass Function and Planetary-mass Object Space Density of the TW HYA Association
DOI: 10.3847/1538-4365/228/2/18 Bibcode: 2017ApJS..228...18G

Weinberger, Alycia J.; Donaldson, Jessica K.; Burgasser, Adam J. +15 more

A determination of the initial mass function (IMF) of the current, incomplete census of the 10 Myr-old TW Hya association (TWA) is presented. This census is built from a literature compilation supplemented with new spectra and 17 new radial velocities from ongoing membership surveys, as well as a reanalysis of Hipparcos data that confirmed HR 4334…

2017 The Astrophysical Journal Supplement Series
Gaia Hipparcos 72
Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades
DOI: 10.1093/mnras/stx1050 Bibcode: 2017MNRAS.471.2882W

Aigrain, S.; Grundahl, F.; Albrecht, S. +20 more

The most powerful tests of stellar models come from the brightest stars in the sky, for which complementary techniques, such as astrometry, asteroseismology, spectroscopy and interferometry, can be combined. The K2 mission is providing a unique opportunity to obtain high-precision photometric time series for bright stars along the ecliptic. Howeve…

2017 Monthly Notices of the Royal Astronomical Society
IUE 72
A Submillimeter Perspective on the GOODS Fields (SUPER GOODS). I. An Ultradeep SCUBA-2 Survey of the GOODS-N
DOI: 10.3847/1538-4357/aa60bb Bibcode: 2017ApJ...837..139C

Wang, W. -H.; Owen, F. N.; Barger, A. J. +3 more

In this first paper in the SUPER GOODS series on powerfully star-forming galaxies in the two GOODS fields, we present a deep SCUBA-2 survey of the GOODS-N at both 850 and 450 µm (central rms noise of 0.28 mJy and 2.6 mJy, respectively). In the central region, the 850 µm observations cover the GOODS-N to near the confusion limit of ∼1.6…

2017 The Astrophysical Journal
Herschel eHST 72
The population of hot subdwarf stars studied with Gaia. I. The catalog of known hot subdwarf stars
DOI: 10.1051/0004-6361/201630135 Bibcode: 2017A&A...600A..50G

Geier, S.; Gänsicke, B. T.; Green, E. M. +5 more

In preparation for the upcoming all-sky data releases of the Gaia mission we compiled a catalog of known hot subdwarf stars and candidates drawn from the literature and yet unpublished databases. The catalog contains 5613 unique sources and provides multi-band photometry from the ultraviolet to the far infrared, ground based proper motions, classi…

2017 Astronomy and Astrophysics
Gaia 72
Multiple stellar populations in Magellanic Cloud clusters - V. The split main sequence of the young cluster NGC 1866
DOI: 10.1093/mnras/stw2965 Bibcode: 2017MNRAS.465.4363M

Anderson, J.; Milone, A. P.; Marino, A. F. +7 more

One of the most unexpected results in the field of stellar populations of the last few years is the discovery that some Magellanic Cloud globular clusters younger than ∼400 Myr exhibit bimodal main sequences (MSs) in their colour-magnitude diagrams (CMDs). Moreover, these young clusters host an extended main-sequence turn-off (eMSTO) in close anal…

2017 Monthly Notices of the Royal Astronomical Society
eHST 72
Coherent Structures at Ion Scales in Fast Solar Wind: Cluster Observations
DOI: 10.3847/1538-4357/aa9022 Bibcode: 2017ApJ...849...49P

Maksimovic, M.; Alexandrova, O.; Lion, S. +5 more

We investigate the nature of magnetic turbulent fluctuations, around ion characteristic scales, in a fast solar wind stream, by using Cluster data. Contrarily to slow solar wind, where both Alfvénic (δ {b}\perp \gg δ {b}\parallel ) and compressive (δ {b}\parallel \gg δ {b}\perp ) coherent structures are …

2017 The Astrophysical Journal
Cluster 72