Search Publications

Detection of H I in Emission in the LYα Emitting Galaxy Haro 11
DOI: 10.3847/0004-6256/152/6/178 Bibcode: 2016AJ....152..178P

Cannon, John M.; Hayes, Matthew; Östlin, Göran +2 more

We present the first robust detection of H I 21 cm emission in the blue compact galaxy Haro 11 using the 100 m Robert C. Byrd Green Bank Telescope (GBT). Haro 11 is a luminous blue compact galaxy with emission in both Lyα and the Lyman continuum. We detect (5.1 ± 0.7 × 108) M of H I gas at an assumed distance of 88 Mpc, mak…

2016 The Astronomical Journal
eHST 14
Chandrayaan-2 dual-frequency SAR: Further investigation into lunar water and regolith
DOI: 10.1016/j.asr.2015.10.029 Bibcode: 2016AdSpR..57..627P

Das, Anup; Putrevu, Deepak; Vachhani, J. G. +2 more

The Space Applications Centre (SAC), one of the major centers of the Indian Space Research Organization (ISRO), is developing a high resolution, dual-frequency Synthetic Aperture Radar as a science payload on Chandrayaan-2, ISRO's second moon mission. With this instrument, ISRO aims to further the ongoing studies of the data from S-band MiniSAR on…

2016 Advances in Space Research
Chandrayaan-1 14
Herschel/HIFI observations of the circumstellar ammonia lines in IRC+10216
DOI: 10.1051/0004-6361/201527290 Bibcode: 2016A&A...592A.131S

Menten, K. M.; Olofsson, H.; Marston, A. P. +14 more

Context. A discrepancy exists between the abundance of ammonia (NH3) derived previously for the circumstellar envelope (CSE) of IRC+10216 from far-IR submillimeter rotational lines and that inferred from radio inversion or mid-infrared (MIR) absorption transitions.
Aims: To address the discrepancy described above…

2016 Astronomy and Astrophysics
Herschel ISO 14
A Search for O2 in CO-depleted Molecular Cloud Cores with Herschel
DOI: 10.3847/0004-637X/830/2/102 Bibcode: 2016ApJ...830..102W

Ceccarelli, Cecilia; Charnley, Steven B.; Cordiner, Martin A. +1 more

The general lack of molecular oxygen in molecular clouds is an outstanding problem in astrochemistry. Extensive searches with the Submillimeter Astronomical Satellite, Odin, and Herschel have only produced two detections; upper limits to the O2 abundance in the remaining sources observed are about 1000 times lower than predicted by chem…

2016 The Astrophysical Journal
Herschel 14
Titan's surface spectra at the Huygens landing site and Shangri-La
DOI: 10.1016/j.icarus.2015.09.016 Bibcode: 2016Icar..270..291R

Le Mouélic, S.; Sotin, C.; D'Aversa, E. +6 more

Titan is an icy satellite of Saturn with a dense atmosphere and covered by a global photochemical organic haze. Ground based observations and the Huygens descent probe allowed to retrieve the main spectral signature of the water ice (Griffith, C.A. et al. [2003]. Science 300(5619), 628-630; Coustenis, A. et al. [2005]. Icarus 177, 89-105) at the s…

2016 Icarus
Huygens 14
Extinction law at a distance up to 25 kpc toward the Galactic poles
DOI: 10.1134/S1063773716070033 Bibcode: 2016AstL...42..445G

Gontcharov, G. A.

Photometry from the Tycho-2, 2MASS, andWISE catalogues for clump and branch giants at a distance up to 25 kpc toward the Galactic poles has allowed the variations of various characteristics of the infrared interstellar extinction law with distance to be analyzed. The results obtained by the extinction law extrapolation method are consistent for di…

2016 Astronomy Letters
Hipparcos 14
Masses of the components of SB2s observed with Gaia - II. Masses derived from PIONIER interferometric observations for Gaia validation
DOI: 10.1093/mnras/stv2497 Bibcode: 2016MNRAS.455.3303H

Mazeh, T.; Grellmann, R.; Tal-Or, L. +15 more

In anticipation of the Gaia astrometric mission, a sample of spectroscopic binaries is being observed since 2010 with the Spectrograph pour l'Observation des PHénomènes des Intérieurs stellaires et des Exoplanètes (SOPHIE) spectrograph at the Haute-Provence Observatory. Our aim is to derive the orbital elements of double-lined spectroscopic binari…

2016 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 14
Radial Distribution of ISM Gas-phase Metallicity in CLASH Clusters at z ~ 0.35: A New Outlook on Environmental Impact on Galaxy Evolution
DOI: 10.3847/0004-637X/831/1/104 Bibcode: 2016ApJ...831..104G

Kewley, Lisa J.; Tran, Kim-Vy H.; Gupta, Anshu +3 more

We present the first observation of cluster-scale radial metallicity gradients from star-forming galaxies. We use DEIMOS on the Keck II telescope to observe two CLASH clusters at z ∼ 0.35: MACS J1115+0129 and RX J1532+3021. Based on our measured interstellar medium properties of star-forming galaxies out to a radius of 2.5 Mpc from the cluster cen…

2016 The Astrophysical Journal
eHST 14
IR excesses around nearby Lambda Boo stars are caused by debris discs rather than ISM bow waves
DOI: 10.1093/mnras/stv2696 Bibcode: 2016MNRAS.456..459D

Wyatt, M. C.; Venn, K. A.; Matthews, B. C. +3 more

Lambda Boo stars are predominately A-type stars with solar abundant C, N, O, and S, but up to 2 dex underabundances of refractory elements. The stars' unusual surface abundances could be due to a selective accretion of volatile gas over dust. It has been proposed that there is a correlation between the Lambda Boo phenomenon and IR excesses which a…

2016 Monthly Notices of the Royal Astronomical Society
Herschel 14
Challenges associated with near-Earth nightside current
DOI: 10.1002/2016JA022948 Bibcode: 2016JGRA..121.6763L

Liemohn, Michael W.; Welling, Daniel T.; Ilie, Raluca +1 more

Every magnetic field of solar and planetary space environments is associated with a current of differentially flowing charged particles. Electric potential patterns in geospace and near other planets are also closely linked with currents. Close to the Earth, particularly in the near-Earth nightside magnetosphere, several current systems wax and wa…

2016 Journal of Geophysical Research (Space Physics)
Cluster 14