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What can We Learn about Solar Coronal Mass Ejections, Coronal Dimmings, and Extreme-ultraviolet Jets through Spectroscopic Observations?
DOI: 10.1088/0004-637X/748/2/106 Bibcode: 2012ApJ...748..106T

He, Jiansen; Wang, Xin; McIntosh, Scott W. +2 more

Solar eruptions, particularly coronal mass ejections (CMEs) and extreme-ultraviolet (EUV) jets, have rarely been investigated with spectroscopic observations. We analyze several data sets obtained by the EUV Imaging Spectrometer on board Hinode and find various types of flows during CMEs and jet eruptions. CME-induced dimming regions are found to …

2012 The Astrophysical Journal
Hinode 108
Supermassive Black Holes, Pseudobulges, and the Narrow-line Seyfert 1 Galaxies
DOI: 10.1088/0004-637X/754/2/146 Bibcode: 2012ApJ...754..146M

Peterson, Bradley M.; Mathur, Smita; Grupe, Dirk +1 more

We present Hubble Space Telescope Advanced Camera for Surveys (ACS) observations of 10 galaxies that host narrow-line Seyfert 1 (NLS1) nuclei, believed to contain relatively smaller mass black holes accreting at high Eddington ratios. We deconvolve each ACS image into a nuclear point source (AGN), a bulge, and a disk, and fitted the bulge with a S…

2012 The Astrophysical Journal
eHST 106
Mid- and Far-infrared Properties of a Complete Sample of Local Active Galactic Nuclei
DOI: 10.1088/0004-637X/754/1/45 Bibcode: 2012ApJ...754...45I

Nakagawa, Takao; Oyabu, Shinki; Gandhi, Poshak +4 more

We investigate the mid- (MIR) to far-infrared (FIR) properties of a nearly complete sample of local active galactic nuclei (AGNs) detected in the Swift/Burst Alert Telescope (BAT) all-sky hard X-ray (14-195 keV) survey, based on the cross correlation with the AKARI infrared survey catalogs complemented by those with Infrared Astronomical Satellite…

2012 The Astrophysical Journal
AKARI Suzaku 106
Hα Equivalent Widths from the 3D-HST Survey: Evolution with Redshift and Dependence on Stellar Mass
DOI: 10.1088/2041-8205/757/2/L22 Bibcode: 2012ApJ...757L..22F

Schmidt, Kasper B.; Franx, Marijn; van Dokkum, Pieter +12 more

We investigate the evolution of the Hα equivalent width, EW(Hα), with redshift and its dependence on stellar mass, using the first data from the 3D-HST survey, a large spectroscopic Treasury program with the Hubble Space Telescope Wide Field Camera 3. Combining our Hα measurements of 854 galaxies at 0.8 < z < 1.5 with those of ground-based s…

2012 The Astrophysical Journal
eHST 106
A Far-ultraviolet Atlas of Low-resolution Hubble Space Telescope Spectra of T Tauri Stars
DOI: 10.1088/0004-637X/744/2/121 Bibcode: 2012ApJ...744..121Y

Herczeg, Gregory J.; Valenti, Jeff A.; Brown, Alexander +6 more

We present a far-ultraviolet (FUV) spectral atlas consisting of spectra of 91 pre-main-sequence stars. Most stars in this sample were observed with the Space Telescope Imaging Spectrograph and Advanced Camera for Surveys on the Hubble Space Telescope (HST). A few archival spectra from the International Ultraviolet Explorer and the Goddard High Res…

2012 The Astrophysical Journal
IUE eHST 106
Can Dust Emission be Used to Estimate the Mass of the Interstellar Medium in Galaxies—A Pilot Project with the Herschel Reference Survey
DOI: 10.1088/0004-637X/761/2/168 Bibcode: 2012ApJ...761..168E

Gear, Walter; Wilson, Christine D.; De Looze, Ilse +23 more

The standard method for estimating the mass of the interstellar medium (ISM) in a galaxy is to use the 21 cm line to trace the atomic gas and the CO 1-0 line to trace the molecular gas. In this paper, we investigate the alternative technique of using the continuum dust emission to estimate the mass of gas in all phases of the ISM. Using Herschel o…

2012 The Astrophysical Journal
Herschel Planck 106
The Role of Streamers in the Deflection of Coronal Mass Ejections: Comparison between STEREO Three-dimensional Reconstructions and Numerical Simulations
DOI: 10.1088/0004-637X/744/1/66 Bibcode: 2012ApJ...744...66Z

Mierla, M.; Poedts, S.; Bemporad, A. +3 more

On 2009 September 21, a filament eruption and the associated coronal mass ejection (CME) were observed by the Solar Terrestrial Relations Observatory (STEREO) spacecraft. The CME originated from the southern hemisphere and showed a deflection of about 15° toward the heliospheric current sheet (HCS) during the propagation in the COR1 field of view.…

2012 The Astrophysical Journal
SOHO 106
Separation of Two Contributions to the High Energy Emission of Cygnus X-1: Polarization Measurements with INTEGRAL SPI
DOI: 10.1088/0004-637X/761/1/27 Bibcode: 2012ApJ...761...27J

Clark, D. J.; Jourdain, E.; Roques, J. P. +1 more

Operational since 2002 on board the INTEGRAL observatory, the SPI spectrometer can be used to perform polarization measurements in the hard X-ray/softγ-ray domain (~130 keV-8 MeV). However, this phenomenon is complex to measure at high energy and requires high fluxes. Cyg X-1 appears to be the best candidate amongst the X-ray binaries since it is …

2012 The Astrophysical Journal
INTEGRAL 105
New Insight into Short-wavelength Solar Wind Fluctuations from Vlasov Theory
DOI: 10.1088/0004-637X/748/2/100 Bibcode: 2012ApJ...748..100S

Belmont, G.; Sahraoui, F.; Goldstein, M. L.

The nature of solar wind (SW) turbulence below the proton gyroscale is a topic that is being investigated extensively nowadays, both theoretically and observationally. Although recent observations gave evidence of the dominance of kinetic Alfvén waves (KAWs) at sub-ion scales with ω < ωci, other studies suggest that the KAW mode cann…

2012 The Astrophysical Journal
Cluster 105
Calibrating 100 Years of Polar Faculae Measurements: Implications for the Evolution of the Heliospheric Magnetic Field
DOI: 10.1088/0004-637X/753/2/146 Bibcode: 2012ApJ...753..146M

DeLuca, Edward E.; Zhang, Jie; Muñoz-Jaramillo, Andrés +1 more

Although the Sun's polar magnetic fields are thought to provide important clues for understanding the 11 year sunspot cycle, including the observed variations of its amplitude and period, the current database of high-quality polar field measurements spans relatively few sunspot cycles. In this paper, we address this deficiency by consolidating Mou…

2012 The Astrophysical Journal
SOHO 105