Search Publications

Star-forming Environments throughout the M101 Group
DOI: 10.3847/1538-4357/aa8fcd Bibcode: 2017ApJ...851...51W

Mihos, J. Christopher; Harding, Paul; Watkins, Aaron E.

We present a multiwavelength study of star formation within the nearby M101 Group, including new deep Hα imaging of M101 and its two companions. We perform a statistical analysis of the Hα-to-FUV flux ratios in H II regions located in three different environments: M101's inner disk, M101's outer disk, and M101's lower-mass companion galaxy NGC 547…

2017 The Astrophysical Journal
eHST 15
Interplanetary Magnetic Flux Ropes as Agents Connecting Solar Eruptions and Geomagnetic Activities
DOI: 10.1007/s11207-017-1204-2 Bibcode: 2017SoPh..292..189M

Marubashi, K.; Cho, K. -S.; Ishibashi, H.

We investigate the solar wind structure for 11 cases that were selected for the campaign study promoted by the International Study of Earth-affecting Solar Transients (ISEST) MiniMax24 Working Group 4. We can identify clear flux rope signatures in nine cases. The geometries of the nine interplanetary magnetic flux ropes (IFRs) are examined with a …

2017 Solar Physics
SOHO 14
A moderately precise dynamical age for the Homunculus of Eta Carinae based on 13 years of HST imaging
DOI: 10.1093/mnras/stx1868 Bibcode: 2017MNRAS.471.4465S

Smith, Nathan

The Hubble Space Telescope archive contains a large collection of images of η Carinae, and this paper analyses those most suitable for measuring its expanding Homunculus Nebula. Multiple intensity tracings through the Homunculus reveal the fractional increase in the overall size of the nebula; this avoids registration uncertainty, mitigates bright…

2017 Monthly Notices of the Royal Astronomical Society
eHST 14
Understanding the nature of the intriguing source X Persei: a deep look with a Suzaku observation
DOI: 10.1093/mnras/stx1281 Bibcode: 2017MNRAS.470..713M

Maitra, Chandreyee; Paul, Biswajit; Pradhan, Pragati +1 more

We present detailed broad-band timing and spectral analysis of the persistent, low luminosity and slowly spinning pulsar X Persei using a deep Suzaku observation of the source. The spectrum is unusually hard with a cyclotron resonance scattering feature (CRSF), the presence of which has been debated. By comparing the spectral models relevant for a…

2017 Monthly Notices of the Royal Astronomical Society
Suzaku 14
IMF dependence of energetic oxygen and hydrogen ion distributions in the near-Earth magnetosphere
DOI: 10.1002/2016JA023471 Bibcode: 2017JGRA..122.5168L

Daly, P. W.; Kronberg, E. A.; Nykyri, K. +5 more

Energetic ion distributions in the near-Earth plasma sheet can provide important information for understanding the entry of ions into the magnetosphere and their transportation, acceleration, and losses in the near-Earth region. In this study, 11 years of energetic proton and oxygen observations (> 274 keV) from Cluster/Research with Adaptive P…

2017 Journal of Geophysical Research (Space Physics)
Cluster 14
Lorentz invariance violation in the neutrino sector: a joint analysis from big bang nucleosynthesis and the cosmic microwave background
DOI: 10.1140/epjc/s10052-017-4959-6 Bibcode: 2017EPJC...77..386D

Cai, Rong-Gen; Guo, Zong-Kuan; Dai, Wei-Ming +1 more

We investigate constraints on Lorentz invariance violation in the neutrino sector from a joint analysis of big bang nucleosynthesis and the cosmic microwave background. The effect of Lorentz invariance violation during the epoch of big bang nucleosynthesis changes the predicted helium-4 abundance, which influences the power spectrum of the cosmic …

2017 European Physical Journal C
Planck 14
Nearby Young, Active, Late-type Dwarfs in Gaia's First Data Release
DOI: 10.3847/1538-4357/aa7065 Bibcode: 2017ApJ...841...73K

Zuckerman, B.; Kastner, Joel H.; Rodriguez, David +3 more

The Galex Nearby Young Star Survey (GALNYSS) has yielded a sample of ∼2000 UV-selected objects that are candidate nearby (D≲ 150 {pc}), young (age ∼ 10-100 Myr), late-type stars. Here, we evaluate the distances and ages of the subsample of (19) GALNYSS stars with Gaia Data Release 1 (DR1) parallax distances D≤slant 120 {pc}. The overall youth of t…

2017 The Astrophysical Journal
Gaia 14
Siriusly, a newly identified intermediate-age Milky Way stellar cluster: a spectroscopic study of Gaia 1
DOI: 10.1093/mnras/stx1892 Bibcode: 2017MNRAS.471.4087S

Bernard, E. J.; Tolstoy, E.; Ferguson, A. M. N. +6 more

We confirm the reality of the recently discovered Milky Way stellar cluster Gaia 1 using spectra acquired with the HERMES and AAOmega spectrographs of the Anglo-Australian Telescope. This cluster had been previously undiscovered due to its close angular proximity to Sirius, the brightest star in the sky at visual wavelengths. Our observations iden…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 14
Emission Lines in the Near-infrared Spectra of the Infrared Quintuplet Stars in the Galactic Center
DOI: 10.3847/1538-4357/aa81d5 Bibcode: 2017ApJ...845..127N

Najarro, F.; Geballe, T. R.; de la Fuente, D. +1 more

We report the detection of a number of emission lines in the 1.0-2.4 µm spectra of four of the five bright-infrared dust-embedded stars at the center of the Galactic center’s (GC) Quintuplet Cluster. Spectroscopy of the central stars of these objects is hampered not only by the large interstellar extinction that obscures all of the objects i…

2017 The Astrophysical Journal
ISO 14
Prominence Eruption Initiated by Helical Kink Instability of an Embedded Flux Rope
DOI: 10.3847/1538-4357/aa9020 Bibcode: 2017ApJ...850...38V

Gopalswamy, N.; Ravindra, B.; Vemareddy, P.

We study the triggering mechanism of a limb-prominence eruption and the associated coronal mass ejection (CME) near AR 12342 using Solar Dynamics Observatory and Large Angle and Spectrometric Coronagraph/Solar Heliospheric Observatory observations. The prominence is seen with an embedded flux thread (FT) at one end and bifurcates from the middle t…

2017 The Astrophysical Journal
SOHO 14