Search Publications

IC 348-SMM2E: a Class 0 proto-brown dwarf candidate forming as a scaled-down version of low-mass stars
DOI: 10.1093/mnras/stu1461 Bibcode: 2014MNRAS.444..833P

Li, Di; Myers, Philip C.; Bouy, Hervé +7 more

We report on Submillimeter Array observations of the 870 µm continuum and CO (3-2), 13CO (2-1), and C18O (2-1) line emission of a faint object, SMM2E, near the driving source of the HH 797 outflow in the IC 348 cluster. The continuum emission shows an unresolved source for which we estimate a mass of gas and dust of 30 …

2014 Monthly Notices of the Royal Astronomical Society
Herschel 62
Detection of Supersonic Downflows and Associated Heating Events in the Transition Region above Sunspots
DOI: 10.1088/2041-8205/789/2/L42 Bibcode: 2014ApJ...789L..42K

Golub, L.; Tian, H.; De Pontieu, B. +18 more

Interface Region Imaging Spectrograph data allow us to study the solar transition region (TR) with an unprecedented spatial resolution of 0.''33. On 2013 August 30, we observed bursts of high Doppler shifts suggesting strong supersonic downflows of up to 200 km s-1 and weaker, slightly slower upflows in the spectral lines Mg II h and k,…

2014 The Astrophysical Journal
IRIS 62
Physical Interpretation of the Angle-dependent Magnetic Helicity Spectrum in the Solar Wind: The Nature of Turbulent Fluctuations near the Proton Gyroradius Scale
DOI: 10.1088/0004-637X/785/2/138 Bibcode: 2014ApJ...785..138K

Klein, Kristopher G.; TenBarge, Jason M.; Howes, Gregory G. +1 more

Motivated by recent observations of distinct parallel and perpendicular signatures in magnetic helicity measurements segregated by wave period and angle between the local magnetic field and the solar wind velocity, this paper undertakes a comparison of three intervals of Ulysses data with synthetic time series generated from a physically motivated…

2014 The Astrophysical Journal
Ulysses 62
A three-dimensional extinction map of the Galactic anticentre from multiband photometry
DOI: 10.1093/mnras/stu1192 Bibcode: 2014MNRAS.443.1192C

Schultheis, M.; Huang, Y.; Chen, B. -Q. +8 more

We present a three-dimensional extinction map in the r band. The map has a spatial angular resolution, depending on latitude, between 3 and 9 arcmin and covers the entire Xuyi Schmidt Telescope Photometric Survey of the Galactic Anticentre (XSTPS-GAC) survey area of over 6000 deg2 for Galactic longitude 140 < l < 240 deg and latit…

2014 Monthly Notices of the Royal Astronomical Society
Planck 62
Ground Level Enhancement in the 2014 January 6 Solar Energetic Particle Event
DOI: 10.1088/2041-8205/790/1/L13 Bibcode: 2014ApJ...790L..13T

Gopalswamy, N.; Davila, J. M.; Yashiro, S. +4 more

We present a study of the 2014 January 6 solar energetic particle event which produced a small ground level enhancement (GLE), making it the second GLE of this unusual solar cycle 24. This event was primarily observed by the South Pole neutron monitors (increase of ~2.5%) while a few other neutron monitors recorded smaller increases. The associate…

2014 The Astrophysical Journal
SOHO 62
Photometric magnetic-activity metrics tested with the Sun: application to Kepler M dwarfs
DOI: 10.1051/swsc/2014011 Bibcode: 2014JSWSC...4A..15M

García, Rafael A.; Mathur, Savita; Salabert, David +1 more

The Kepler mission has been providing high-quality photometric data leading to many breakthroughs in the exoplanet search and in stellar physics. Stellar magnetic activity results from the interaction between rotation, convection, and magnetic field. Constraining these processes is important if we want to better understand stellar magnetic activit…

2014 Journal of Space Weather and Space Climate
SOHO 62
Fluctuations and Flares in the Ultraviolet Line Emission of Cool Stars: Implications for Exoplanet Transit Observations
DOI: 10.1088/0067-0049/211/1/9 Bibcode: 2014ApJS..211....9L

Loyd, R. O. Parke; France, Kevin

Variations in stellar flux can potentially overwhelm the photometric signal of a transiting planet. Such variability has not previously been well-characterized in the ultraviolet lines used to probe the inflated atmospheres surrounding hot Jupiters. Therefore, we surveyed 38 F-M stars for intensity variations in four narrow spectroscopic bands: tw…

2014 The Astrophysical Journal Supplement Series
eHST 62
Possible Detection of the Stellar Donor or Remnant for the Type Iax Supernova 2008ha
DOI: 10.1088/0004-637X/792/1/29 Bibcode: 2014ApJ...792...29F

Foley, Ryan J.; Rest, Armin; Fong, Wen-fai +5 more

Type Iax supernovae (SNe Iax) are thermonuclear explosions that are related to SNe Ia, but are physically distinct. The most important differences are that SNe Iax have significantly lower luminosity (1%-50% that of typical SNe Ia), lower ejecta mass (~0.1-0.5 M ), and may leave a bound remnant. The most extreme SN Iax is SN 2008ha, wh…

2014 The Astrophysical Journal
eHST 62
The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115: Witnessing the Flow of Hot Gas within the Bondi Radius
DOI: 10.1088/0004-637X/780/1/9 Bibcode: 2014ApJ...780....9W

Bregman, Joel N.; Wong, Ka-Wah; Irwin, Jimmy A. +3 more

Observational confirmation of hot accretion model predictions has been hindered by the challenge to resolve spatially the Bondi radii of black holes with X-ray telescopes. Here, we use the Megasecond Chandra X-ray Visionary Project observation of the NGC 3115 supermassive black hole to place the first direct observational constraints on the spatia…

2014 The Astrophysical Journal
eHST 62
Neutral interstellar He parameters in front of the heliosphere 1994-2007
DOI: 10.1051/0004-6361/201424127 Bibcode: 2014A&A...569A...8B

Bzowski, M.; Witte, M.; Banaszkiewicz, M. +3 more

Context. A recent analysis of IBEX measurements of the neutral interstellar He flux showed that the inflow velocity vector is different from the results of an earlier analysis of observations from the GAS instrument onboard Ulysses. A recently published compilation of published results on the helium inflow direction from the past ~40 years suggest…

2014 Astronomy and Astrophysics
Ulysses 62