Search Publications

Impact of solar EUV flux on CO Cameron band and CO2+ UV doublet emissions in the dayglow of Mars
DOI: 10.1016/j.pss.2011.08.010 Bibcode: 2012P&SS...63..110J

Bhardwaj, Anil; Jain, Sonal Kumar

This study is aimed at making a calculation about the impact of the two most commonly used solar EUV flux models - SOLAR2000 (S2K) of Tobiska (2004) and EUVAC model of Richards et al. (1994) - on photoelectron fluxes, volume emission rates, ion densities and CO Cameron and CO2+ UV doublet band dayglow emissions on Mars in thr…

2012 Planetary and Space Science
MEx 30
On the Relationship between the Coronal Magnetic Decay Index and Coronal Mass Ejection Speed
DOI: 10.1088/0004-637X/761/1/52 Bibcode: 2012ApJ...761...52X

Xu, Yan; Liu, Chang; Jing, Ju +1 more

Numerical simulations suggest that kink and torus instabilities are two potential contributors to the initiation and prorogation of eruptive events. A magnetic parameter called the decay index (i.e., the coronal magnetic gradient of the overlying fields above the eruptive flux ropes) could play an important role in controlling the kinematics of er…

2012 The Astrophysical Journal
SOHO 30
Interferometric CO(3-2) Observations toward the Central Region of NGC 1068
DOI: 10.1088/0004-637X/746/2/129 Bibcode: 2012ApJ...746..129T

Matsushita, Satoki; Hwang, Chorng-Yuan; Espada, Daniel +2 more

We present CO(3-2) interferometric observations of the central region of the Seyfert 2 galaxy NGC 1068 using the Submillimeter Array, together with CO(1-0) data taken with the Owens Valley Radio Observatory Millimeter Array. Both the CO(3-2) and CO(1-0) emission lines are mainly distributed within ~5 arcsec of the nucleus and along the spiral arms…

2012 The Astrophysical Journal
eHST 30
NGC 5548: Lack of a Broad Fe Kα Line and Constraints on the Location of the Hard X-Ray Source
DOI: 10.1088/0004-637X/744/1/13 Bibcode: 2012ApJ...744...13B

Liu, Y.; Elvis, M.; Krongold, Y. +2 more

We present an analysis of the co-added and individual 0.7-40 keV spectra from seven Suzaku observations of the Sy 1.5 galaxy NGC 5548 taken over a period of eight weeks. We conclude that the source has a moderately ionized, three-zone warm absorber, a power-law continuum, and exhibits contributions from cold, distant reflection. Relativistic refle…

2012 The Astrophysical Journal
Suzaku 30
Thermal infrared properties of classical and type II Cepheids. Diffraction limited 10 µm imaging with VLT/VISIR
DOI: 10.1051/0004-6361/201117307 Bibcode: 2012A&A...538A..24G

Kervella, P.; Mérand, A.; Gallenne, A.

We present new thermal infrared (IR) photometry and spectral energy distributions (SEDs) of eight classical Cepheids (type I) and three type II Cepheids, using VISIR thermal IR photometric measurements, supplemented with literature data. We used the BURST mode of the instrument to get diffraction-limited images at 8.59, 11.25, and 11.85 µm. …

2012 Astronomy and Astrophysics
AKARI 30
Discovery of Variability of the Progenitor of SN 2011dh in M 51 Using the Large Binocular Telescope
DOI: 10.1088/0004-637X/747/1/23 Bibcode: 2012ApJ...747...23S

Kochanek, C. S.; Stanek, K. Z.; Gerke, J. R. +1 more

We show that the candidate progenitor of the core-collapse SN 2011dh in M 51 (8 Mpc away) was fading by 0.039 ± 0.006 mag yr-1 during the 3 years prior to the supernova, and that this level of variability is moderately unusual for other similar stars in M 51. While there are uncertainties about whether the true progenitor was a blue com…

2012 The Astrophysical Journal
eHST 30
Metallicities of Emission-line Galaxies from HST ACS PEARS and HST WFC3 ERS Grism Spectroscopy at 0.6 < z < 2.4
DOI: 10.1088/0004-6256/144/1/28 Bibcode: 2012AJ....144...28X

Pirzkal, Nor; Cohen, Seth; Windhorst, Rogier A. +9 more

Galaxies selected on the basis of their emission-line strength show low metallicities, regardless of their redshifts. We conclude this from a sample of faint galaxies at redshifts between 0.6 < z < 2.4, selected by their prominent emission lines in low-resolution grism spectra in the optical with the Advanced Camera for Surveys on the Hubble…

2012 The Astronomical Journal
eHST 30
A superburst candidate in EXO 1745-248 as a challenge to thermonuclear ignition models
DOI: 10.1111/j.1365-2966.2012.21769.x Bibcode: 2012MNRAS.426..927A

Altamirano, D.; Degenaar, N.; Wijnands, R. +6 more

We report on Chandra, Rossi X-ray Timing Explorer (RXTE), Swift/Burst Alert Telescope (BAT) and MAXI observations of an X-ray flare of ∼1 d and subsequent outburst of a transient X-ray source observed in 2011 October-November in the globular cluster Terzan 5. We show that the source is the same as the transient that was active in 2000, i.e. the ne…

2012 Monthly Notices of the Royal Astronomical Society
INTEGRAL 30
The peculiar 2011 outburst of the black hole candidate IGR J17091-3624, a GRS 1915+105-like source?
DOI: 10.1111/j.1365-2966.2012.20834.x Bibcode: 2012MNRAS.422.3130C

Capitanio, F.; Ferrigno, C.; Bozzo, E. +3 more

We report on the long-term monitoring campaign of the black hole candidate IGR J17091-3624 performed with INTEGRAL and Swift during the peculiar outburst started on 2011 January. We have studied the two-month spectral evolution of the source in detail. Unlike the previous outbursts, the initial transition from the hard to the soft state in 2011 wa…

2012 Monthly Notices of the Royal Astronomical Society
INTEGRAL 30
Mergers and interactions in Sloan Digital Sky Survey type 2 quasars at z∼ 0.3-0.4. SDSS J143027.66-005614.8: a case study
DOI: 10.1111/j.1365-2966.2012.20652.x Bibcode: 2012MNRAS.423...80V

Villar-Martín, M.; Rose, M.; Cabrera Lavers, A. +3 more

We present a compilation of Hubble Space Telescope (HST) images of 58 luminous Sloan Digital Sky Survey (SDSS) type 2 active galactic nuclei (AGNs) at ?. Of these, 42 are type 2 quasars, which is a good representation of all optically selected SDSS type 2 quasars in this z range. We find that the majority of the host galaxies are ellipticals (30/4…

2012 Monthly Notices of the Royal Astronomical Society
eHST 30