Search Publications

Suzaku broad-band spectroscopy of RX J1347.5-1145: constraints on the extremely hot gas and non-thermal emission
DOI: 10.1051/0004-6361:200810122 Bibcode: 2008A&A...491..363O

Yoshikawa, K.; Ota, N.; Komatsu, E. +6 more

Context: We present the results of our analysis of long Suzaku observations (149 ks and 122 ks for XIS and HXD, respectively) of the most X-ray luminous galaxy cluster, RX J1347.5-1145, at z=0.451.
Aims: To understand the gas physics of a violent, cluster merger, we study physical properties of the hot ( 20 keV) gas clump in the south-east (SE…

2008 Astronomy and Astrophysics
Suzaku XMM-Newton 39
A New H I Survey of Active Galaxies
DOI: 10.1086/588217 Bibcode: 2008ApJS..177..103H

Ho, Luis C.; Greene, Jenny E.; Darling, Jeremy

We have conducted a new Arecibo survey for H I emission for 113 galaxies with broad-line (type 1) active galactic nuclei (AGNs) out to recession velocities as high as ~35,000 km s-1. The primary aim of the study is to obtain sensitive H I spectra for a well-defined, uniformly selected sample of active galaxies that have estimates of the…

2008 The Astrophysical Journal Supplement Series
eHST 39
Strongly Blueshifted Phenomena Observed with Hinode EIS in the 2006 December 13 Solar Flare
DOI: 10.1086/590419 Bibcode: 2008ApJ...685..622A

Culhane, J. L.; Hara, Hirohisa; Narukage, Noriyuki +5 more

We present a detailed examination of strongly blueshifted emission lines observed with the EUV Imaging Spectrometer on board the Hinode satellite. We found two kinds of blueshifted phenomenon associated with the X3.4 flare that occurred on 2006 December 13. One was related to a plasmoid ejection seen in soft X-rays. It was very bright in all the l…

2008 The Astrophysical Journal
Hinode 39
Distribution of the ultraviolet nitric oxide Martian night airglow: Observations from Mars Express and comparisons with a one-dimensional model
DOI: 10.1029/2007JE003037 Bibcode: 2008JGRE..113.8012C

Reberac, A.; Bertaux, J. -L.; Leblanc, F. +4 more

Limb observations with the SPICAM ultraviolet spectrometer on board the Mars Express orbiter revealed ultraviolet nightglow emission in the δ (190-240 nm) and γ (225-270 nm) bands of nitric oxide. This emission arises from radiative recombination between O(3P) and N(4S) atoms that are produced on the day side and form excited…

2008 Journal of Geophysical Research (Planets)
MEx 39
How rapidly do neutron stars spin at birth? Constraints from archival X-ray observations of extragalactic supernovae
DOI: 10.1111/j.1365-2966.2007.12821.x Bibcode: 2008MNRAS.384.1638P

Soria, Roberto; Stella, Luigi; Perna, Rosalba +1 more

Traditionally, studies aimed at inferring the distribution of birth periods of neutron stars are based on radio surveys. Here we propose an independent method to constrain the pulsar spin periods at birth based on their X-ray luminosities. In particular, the observed luminosity distribution of supernovae (SNe) poses a constraint on the initial rot…

2008 Monthly Notices of the Royal Astronomical Society
XMM-Newton 39
HST ACS Imaging of M82: A Comparison of Mass and Size Distribution Functions of the Younger Nuclear and Older Disk Clusters
DOI: 10.1086/587541 Bibcode: 2008ApJ...679..404M

Luna, A.; Mayya, Y. D.; Rosa-González, D. +3 more

We present the results obtained from an objective search for stellar clusters, both in the currently active nuclear starburst region, and in the poststarburst disk of M82. Images obtained with the Advanced Camera for Surveys (ACS) on board the Hubble Space Telescope (HST) in F435W (B), F555W (V), and F814W (I) filters were used in the search for t…

2008 The Astrophysical Journal
eHST 39
On the radial distribution of white dwarfs in the globular cluster NGC 6397
DOI: 10.1111/j.1745-3933.2007.00402.x Bibcode: 2008MNRAS.383L..20D

Anderson, J.; Davis, D. S.; King, I. R. +5 more

We have examined the radial distribution of white dwarfs over a single Hubble Space Telescope/Advanced Camera for Surveys field in the nearby globular cluster NGC 6397. In relaxed populations, such as in a globular cluster, stellar velocity dispersion, and hence radial distribution, is directly dependent on stellar masses. The progenitors of very …

2008 Monthly Notices of the Royal Astronomical Society
eHST 39
A Search for Molecular Gas in the Nucleus of M87 and Implications for the Fueling of Supermassive Black Holes
DOI: 10.1086/592592 Bibcode: 2008ApJ...689..775T

Beuther, Henrik; Walter, Fabian; Tan, Jonathan C. +1 more

Supermassive black holes in giant elliptical galaxies are remarkably faint given their expected accretion rates. This motivates models of radiatively inefficient accretion due to either ion-electron thermal decoupling, generation of outflows that inhibit accretion, or settling of gas to a gravitationally unstable disk that forms stars in preferenc…

2008 The Astrophysical Journal
eHST 39
Observations of the north polar water ice annulus on Mars using THEMIS and TES
DOI: 10.1016/j.pss.2007.08.008 Bibcode: 2008P&SS...56..256W

Bandfield, Joshua L.; Castaño, Rebecca; Titus, Timothy N. +2 more

The Martian seasonal CO2 ice caps advance and retreat each year. In the spring, as the CO2 cap gradually retreats, it leaves behind an extensive defrosting zone from the solid CO2 cap to the location where all CO2 frost has sublimated. We have been studying this phenomenon in the north polar region using…

2008 Planetary and Space Science
MEx 39
Emission from Very Small Grains and PAH Molecules in Monte Carlo Radiation Transfer Codes: Application to the Edge-On Disk of Gomez's Hamburger
DOI: 10.1086/592185 Bibcode: 2008ApJ...688.1118W

Wood, Kenneth; Robitaille, Thomas; Draine, Bruce T. +1 more

We have modeled optical to far-infrared images, photometry, and spectroscopy of the object known as Gomez's Hamburger. We reproduce the images and spectrum with an edge-on disk of mass 0.3 M and radius 1600 AU, surrounding an A0 III star at a distance of 280 pc. Our mass estimate is in excellent agreement with recent CO observations. H…

2008 The Astrophysical Journal
eHST 39