Search Publications

Understanding the Physical Nature of Coronal "EIT Waves"
DOI: 10.1007/s11207-016-1030-y Bibcode: 2017SoPh..292....7L

Long, D. M.; Veronig, A. M.; Vršnak, B. +9 more

For almost 20 years the physical nature of globally propagating waves in the solar corona (commonly called "EIT waves") has been controversial and subject to debate. Additional theories have been proposed over the years to explain observations that did not agree with the originally proposed fast-mode wave interpretation. However, the incompatibili…

2017 Solar Physics
PROBA-2 SOHO 87
LACEwING: A New Moving Group Analysis Code
DOI: 10.3847/1538-3881/153/3/95 Bibcode: 2017AJ....153...95R

Blunt, Sarah C.; Faherty, Jacqueline K.; Cruz, Kelle L. +3 more

We present a new nearby young moving group (NYMG) kinematic membership analysis code, LocAting Constituent mEmbers In Nearby Groups (LACEwING), a new Catalog of Suspected Nearby Young Stars, a new list of bona fide members of moving groups, and a kinematic traceback code. LACEwING is a convergence-style algorithm with carefully vetted membership s…

2017 The Astronomical Journal
Gaia 86
The Herschel Orion Protostar Survey: Luminosity and Envelope Evolution
DOI: 10.3847/1538-4357/aa6d69 Bibcode: 2017ApJ...840...69F

Manoj, P.; Myers, Philip C.; Fischer, William J. +12 more

The Herschel Orion Protostar Survey obtained well-sampled 1.2-870 µm spectral energy distributions (SEDs) of over 300 protostars in the Orion molecular clouds, home to most of the young stellar objects (YSOs) in the nearest 500 pc. We plot the bolometric luminosities and temperatures for 330 Orion YSOs, 315 of which have bolometric temperatu…

2017 The Astrophysical Journal
Herschel 86
Measurements of Physical Parameters of White Dwarfs: A Test of the Mass-Radius Relation
DOI: 10.3847/1538-4357/aa8bb6 Bibcode: 2017ApJ...848...11B

Fontaine, G.; Bergeron, P.; Bédard, A.

We present a detailed spectroscopic and photometric analysis of 219 DA and DB white dwarfs for which trigonometric parallax measurements are available. Our aim is to compare the physical parameters derived from the spectroscopic and photometric techniques, and then to test the theoretical mass-radius relation for white dwarfs using these results. …

2017 The Astrophysical Journal
Gaia 86
Magnifying the Early Episodes of Star Formation: Super Star Clusters at Cosmological Distances
DOI: 10.3847/1538-4357/aa74ae Bibcode: 2017ApJ...842...47V

Castellano, M.; Pentericci, L.; Vignali, C. +27 more

We study the spectrophotometric properties of a highly magnified (µ ≃ 40{--}70) pair of stellar systems identified at z = 3.2222 behind the Hubble Frontier Field galaxy cluster MACS J0416. Five multiple images (out of six) have been spectroscopically confirmed by means of VLT/MUSE and VLT/X-Shooter observations. Each image includes two faint…

2017 The Astrophysical Journal
eHST 86
The Rosetta mission orbiter science overview: the comet phase
DOI: 10.1098/rsta.2016.0262 Bibcode: 2017RSPTA.37560262T

Buratti, B. J.; Altobelli, N.; Taylor, M. G. G. T. +1 more

The international Rosetta mission was launched in 2004 and consists of the orbiter spacecraft Rosetta and the lander Philae. The aim of the mission is to map the comet 67P/Churyumov-Gerasimenko by remote sensing, and to examine its environment in situ and its evolution in the inner Solar System. Rosetta was the first spacecraft to rendezvous with …

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta 86
Chromosphere to 1 AU Simulation of the 2011 March 7th Event: A Comprehensive Study of Coronal Mass Ejection Propagation
DOI: 10.3847/1538-4357/834/2/172 Bibcode: 2017ApJ...834..172J

de Koning, C. A.; Gombosi, T. I.; Tóth, G. +5 more

We perform and analyze the results of a global magnetohydrodynamic simulation of the fast coronal mass ejection (CME) that occurred on 2011 March 7. The simulation is made using the newly developed Alfvén Wave Solar Model (AWSoM), which describes the background solar wind starting from the upper chromosphere and extends to 24 R. Coupli…

2017 The Astrophysical Journal
SOHO 85
The Greater Taurus-Auriga Ecosystem. I. There is a Distributed Older Population
DOI: 10.3847/1538-4357/aa62a0 Bibcode: 2017ApJ...838..150K

Herczeg, Gregory J.; Rizzuto, Aaron C.; Kraus, Adam L. +5 more

The census of Taurus-Auriga has been assembled over seven decades and inherited the biases and incompleteness of the input studies. The unusual shape of its inferred initial mass function (IMF) and the existence of isolated disk-bearing stars suggest that additional (likely disk-free) members remain to be discovered. We therefore have begun a glob…

2017 The Astrophysical Journal
Gaia 85
Space Telescope and Optical Reverberation Mapping Project.VI. Reverberating Disk Models for NGC 5548
DOI: 10.3847/1538-4357/835/1/65 Bibcode: 2017ApJ...835...65S

Im, M.; Geier, S.; Zheng, W. +90 more

We conduct a multiwavelength continuum variability study of the Seyfert 1 galaxy NGC 5548 to investigate the temperature structure of its accretion disk. The 19 overlapping continuum light curves (1158 \mathringA to 9157 \mathringA ) combine simultaneous Hubble Space Telescope, Swift, and ground-based observations over a 180 day period from 2014 J…

2017 The Astrophysical Journal
eHST 85
In-orbit Performance of UVIT and First Results
DOI: 10.1007/s12036-017-9445-x Bibcode: 2017JApA...38...28T

Stalin, C. S.; Rao, N. Kameswara; Sutaria, F. +23 more

The performance of the ultraviolet telescope (UVIT) on-board AstroSat is reported. The performance in orbit is also compared with estimates made from the calibrations done on the ground. The sensitivity is found to be within 15% of the estimates, and the spatial reso…

2017 Journal of Astrophysics and Astronomy
eHST 85