Search Publications

NuSTAR and XMM-Newton Observations of 1E1743.1-2843: Indications of a Neutron Star LMXB Nature of the Compact Object
DOI: 10.3847/0004-637X/822/1/57 Bibcode: 2016ApJ...822...57L

Hailey, Charles J.; Mori, Kaya; Zhang, Shuo +13 more

We report on the results of NuSTAR and XMM-Newton observations of the persistent X-ray source 1E1743.1-2843, located in the Galactic Center region. The source was observed between 2012 September and October by NuSTAR and XMM-Newton, providing almost simultaneous observations in the hard and soft X-ray bands. The high X-ray luminosity points to the…

2016 The Astrophysical Journal
XMM-Newton 10
The Kinematics of the Nebular Shells Around Low Mass Progenitors of PNe with Low Metallicity
DOI: 10.3847/0004-6256/151/3/53 Bibcode: 2016AJ....151...53P

Richer, Michael G.; López, José Alberto; Pereyra, Margarita

We analyze the internal kinematics of 26 planetary nebulae (PNe) with low metallicity that appear to derive from progenitor stars of the lowest masses, including the halo PN population. Based upon spatially resolved, long-slit, echelle spectroscopy drawn from the San Pedro Mártir Kinematic Catalog of PNe, we characterize the kinematics of these PN…

2016 The Astronomical Journal
eHST 10
Stellar classification of CoRoT targets
DOI: 10.1051/0004-6361/201628627 Bibcode: 2016A&A...595A..95D

Deeg, H.; Deleuil, M.; Moutou, C. +4 more

Context. The CoRoT mission was the first dedicated to the search for exoplanets from space. The CoRoT exoplanet channel observed about 163 600 targets to detect transiting planetary companions. In addition to the search for exoplanets, the extremely precise photometric time series provided by CoRoT for this vast number of stars is an invaluable re…

2016 Astronomy and Astrophysics
CoRoT 10
High-angular-resolution stellar imaging with occultations from the Cassini spacecraft - III. Mira
DOI: 10.1093/mnras/stw045 Bibcode: 2016MNRAS.457.1410S

Nicholson, Philip D.; Hedman, Matthew M.; Stewart, Paul N. +1 more

We present an analysis of spectral and spatial data of Mira obtained by the Cassini spacecraft, which not only observed the star's spectra over a broad range of near-infrared wavelengths, but was also able to obtain high-resolution spatial information by watching the star pass behind Saturn's rings. The observed spectral range of 1-5 microns revea…

2016 Monthly Notices of the Royal Astronomical Society
Cassini 10
The VIRUS-P Exploration of Nearby Galaxies (VENGA): Radial Gas Inflow and Shock Excitation in NGC 1042
DOI: 10.3847/0004-637X/823/2/85 Bibcode: 2016ApJ...823...85L

Blanc, Guillermo A.; Jogee, Shardha; Luo, Rongxin +3 more

NGC 1042 is a late-type bulgeless disk galaxy that hosts low-luminosity active galactic nuclei (AGNs) coincident with a massive nuclear star cluster. In this paper, we present the integral field spectroscopy studies of this galaxy, based on the data obtained with the Mitchell spectrograph on the 2.7 m Harlan J. Smith telescope. In the central 100-…

2016 The Astrophysical Journal
eHST 10
Contamination in electron observations of the silicon detector on board Cluster/RAPID/IES instrument in Earth's radiation belts and ring current
DOI: 10.1002/2016SW001369 Bibcode: 2016SpWea..14..449K

Daly, P. W.; Klecker, B.; Pierrard, V. +10 more

Since more than 15 years, the Cluster mission passes through Earth's radiation belts at least once every 2 days for several hours, measuring the electron intensity at energies from 30 to 400 keV. These data have previously been considered not usable due to contamination caused by penetrating energetic particles (protons at >100 keV and electron…

2016 Space Weather
Cluster 10
The Putative Old, Nearby Cluster Lodén 1 Does Not Exist
DOI: 10.3847/0004-6256/152/1/7 Bibcode: 2016AJ....152....7H

Wright, Jason T.; Curtis, Jason L.; Han, Eunkyu

Astronomers have access to precious few nearby, middle-aged benchmark star clusters. Within 500 pc, there are only NGC 752 and Ruprecht 147 (R147) at 1.5 and 3 Gyr, respectively. The Database for Galactic Open Clusters (WEBDA) also lists Lodén 1 as a 2 Gyr cluster at a distance of 360 pc. If this is true, Lodén 1 could become a useful benchmark cl…

2016 The Astronomical Journal
Hipparcos 10
The Star Cluster Mass-Galactocentric Radius Relation: Implications for Cluster Formation
DOI: 10.3847/0004-637X/816/1/9 Bibcode: 2016ApJ...816....9S

Fan, Zhou; de Grijs, Richard; Cameron, Ewan +1 more

Whether or not the initial star cluster mass function is established through a universal, galactocentric-distance-independent stochastic process, on the scales of individual galaxies, remains an unsolved problem. This debate has recently gained new impetus through the publication of a study that concluded that the maximum cluster mass in a given p…

2016 The Astrophysical Journal
eHST 10
Rosetta mission operations for landing
DOI: 10.1016/j.actaastro.2016.01.013 Bibcode: 2016AcAau.125...30A

Accomazzo, Andrea; Lodiot, Sylvain; Companys, Vicente

The International Rosetta Mission of the European Space Agency (ESA) was launched on 2nd March 2004 on its 10 year journey to comet Churyumov-Gerasimenko and has reached it early August 2014. The main mission objectives were to perform close observations of the comet nucleus throughout its orbit around the Sun and deliver the lander Philae to its …

2016 Acta Astronautica
Rosetta 10
Constraining the escape fraction of ionizing photons from H II regions within NGC 300: A concept paper
DOI: 10.1051/0004-6361/201527819 Bibcode: 2016A&A...592A..47N

Bastian, N.; Niederhofer, F.; Hilker, M. +1 more

Using broadband photometry from the Hubble Space Telescope in combination with Very Large Telescope narrowband Hα observations of the nearby spiral galaxy NGC 300, we explore a method for estimating the escape fractions of hydrogen-ionizing photons from H II regions within this galaxy. Our goal in this concept study is to evaluate the spectral typ…

2016 Astronomy and Astrophysics
eHST 10