Search Publications

X-Ray-Emitting Stars Identified from the ROSAT All-Sky Survey and the Sloan Digital Sky Survey
DOI: 10.1088/0067-0049/181/2/444 Bibcode: 2009ApJS..181..444A

Anderson, Scott F.; Hawley, Suzanne L.; Szkody, Paula +7 more

The ROSAT All-Sky Survey (RASS) was the first imaging X-ray survey of the entire sky. Combining the RASS Bright and Faint Source Catalogs yields an average of about three X-ray sources per square degree. However, while X-ray source counterparts are known to range from distant quasars to nearby M dwarfs, the RASS data alone are often insufficient t…

2009 The Astrophysical Journal Supplement Series
XMM-Newton 53
Propagating transverse waves in soft X-ray coronal jets
DOI: 10.1051/0004-6361/200911840 Bibcode: 2009A&A...498L..29V

Nakariakov, V. M.; Verwichte, E.; Van Doorsselaere, T. +1 more

Aims: The theoretical model for magnetohydrodynamic (MHD) modes guided by a field-aligned plasma cylinder with a steady flow is adapted to interpret transverse waves observed in solar coronal hot jets, discovered with Hinode/XRT in terms of fast magnetoacoustic kink modes.
Methods: Dispersion relations for linear magnetoacoustic perturbations …

2009 Astronomy and Astrophysics
Hinode 53
Feedback through multiple outbursts in the cluster 2A 0335+096
DOI: 10.1111/j.1365-2966.2009.14892.x Bibcode: 2009MNRAS.396.1449S

Fabian, A. C.; Sanders, J. S.; Taylor, G. B.

We examine the core of the X-ray bright galaxy cluster 2A 0335+096 using deep Chandra X-ray imaging and spatially resolved spectroscopy, and include new radio observations. The set of around eight X-ray bright blobs in the core of the cluster, appearing like eggs in a bird's nest, contains multiphase gas from ~0.5 to 2 keV. The morphology of the c…

2009 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 53
The Ultraviolet Spectrum and Physical Properties of the Mass Donor Star in HD 226868 = Cygnus X-1
DOI: 10.1088/0004-637X/701/2/1895 Bibcode: 2009ApJ...701.1895C

Kaper, L.; Herrero, A.; Bolton, C. T. +8 more

We present an examination of high-resolution, ultraviolet (UV) spectroscopy from Hubble Space Telescope of the photospheric spectrum of the O-supergiant in the massive X-ray binary HD 226868 = Cyg X-1. We analyzed this and ground-based optical spectra to determine the effective temperature and gravity of the O9.7 Iab supergiant. Using non-LTE, lin…

2009 The Astrophysical Journal
IUE eHST 53
Cassini RADAR images at Hotei Arcus and western Xanadu, Titan: Evidence for geologically recent cryovolcanic activity
DOI: 10.1029/2008GL036415 Bibcode: 2009GeoRL..36.4203W

Lorenz, R. D.; Janssen, M. A.; Lunine, J. I. +14 more

Images obtained by the Cassini Titan Radar Mapper (RADAR) reveal lobate, flowlike features in the Hotei Arcus region that embay and cover surrounding terrains and channels. We conclude that they are cryovolcanic lava flows younger than surrounding terrain, although we cannot reject the sedimentary alternative. Their appearance is grossly similar t…

2009 Geophysical Research Letters
Cassini 53
Sizes of LYα-emitting Galaxies and Their Rest-frame Ultraviolet Components at z = 3.1
DOI: 10.1088/0004-637X/705/1/639 Bibcode: 2009ApJ...705..639B

Schawinski, Kevin; Gronwall, Caryl; Gawiser, Eric +3 more

We present a rest-frame ultraviolet analysis of ~120 z ~ 3.1 Lyman Alpha Emitters (LAEs) in the Extended Chandra Deep Field South. Using Hubble Space Telescope (HST) images taken as part of the Galaxy Evolution From Morphology and SEDS (GEMS) survey, Great Observatories Origins Deep Survey (GOODS), and Hubble Ultradeep Field surveys, we analyze th…

2009 The Astrophysical Journal
eHST 53
Suzaku Observations of Tycho's Supernova Remnant
DOI: 10.1093/pasj/61.sp1.S167 Bibcode: 2009PASJ...61S.167T

Kunieda, Hideyo; Szymkowiak, Andrew; Kokubun, Motohide +19 more

Tycho's supernova remnant was observed by the XIS and HXD instruments onboard the Suzaku satellite on 2006 June 26--29 for 92ks. The spectrum up to 30keV was well fitted with a two-component model, consisting of a power-law with a photon index of 2.7 and a thermal bremsstrahlung model with a temperature of 4.7keV. The former component can alternat…

2009 Publications of the Astronomical Society of Japan
Suzaku 53
The ACS Nearby Galaxy Survey Treasury. II. Young Stars and their Relation to Hα and UV Emission Timescales in the M81 Outer Disk
DOI: 10.1088/0004-637X/691/1/115 Bibcode: 2009ApJ...691..115G

de Jong, Roelof S.; Williams, Benjamin F.; Dolphin, Andrew +11 more

We have obtained resolved stellar photometry from Hubble Space Telescope Advanced Camera for Surveys observations of a field in the outer disk of M81 as part of ANGST. Motivated by the recent discovery of extended UV disks around many nearby spiral galaxies, we use the observed stellar population to derive the recent star formation histories of fi…

2009 The Astrophysical Journal
eHST 53
IGR J17544-2619 in Depth With Suzaku: Direct Evidence for Clumpy Winds in a Supergiant Fast X-ray Transient
DOI: 10.1088/0004-637X/707/1/243 Bibcode: 2009ApJ...707..243R

Smith, David M.; Negueruela, Ignacio; Rampy, Rachel A.

We present direct evidence for dense clumps of matter in the companion wind in a Supergiant Fast X-ray Transient (SFXT) binary. This is seen as a brief period of enhanced absorption during one of the bright, fast flares that distinguish these systems. The object under study was IGR J17544-2619, and a total of 236 ks of data were accumulated with t…

2009 The Astrophysical Journal
Suzaku 53
Modelling the Longitudinal Asymmetry in Sunspot Emergence: The Role of the Wilson Depression
DOI: 10.1007/s11207-009-9420-z Bibcode: 2009SoPh..260....5W

Watson, F.; Fletcher, L.; Dalla, S. +1 more

The distributions of sunspot longitude at first appearance and at disappearance display an east-west asymmetry that results from a reduction in visibility as one moves from disk centre to the limb. To first order, this is explicable in terms of simple geometrical foreshortening. However, the centre-to-limb visibility variation is much larger than …

2009 Solar Physics
SOHO 53