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A Multi-Wavelength Investigation of the Unidentified Gamma-Ray Source HESS J1708-410
DOI: 10.1088/0004-637X/707/2/1717 Bibcode: 2009ApJ...707.1717V

Funk, Stefan; Hinton, Jim; Van Etten, Adam

We report on recent XMM-Newton observations, archival radio continuum and CO data, and spectral energy distribution (SED) modeling of the unidentified Galactic plane source HESS J1708-410. No significant extended X-ray emission is observed, and we place an upper limit of 3.2 × 10-13 erg cm-2 s-1 in the 2-4 keV rang…

2009 The Astrophysical Journal
XMM-Newton 6
Clustering of Red Galaxies Around the z = 1.53 Quasar 3C 270.1
DOI: 10.1088/0004-637X/695/1/724 Bibcode: 2009ApJ...695..724H

Wilkes, Belinda J.; Fazio, G. G.; Ashby, M. L. N. +6 more

In the paradigm of hierarchical galaxy formation, luminous radio galaxies mark mass assembly peaks that should contain clusters of galaxies. Observations of the z = 1.53 quasar 3C 270.1 with the Spitzer Space Telescope at 3.6-24 µm and with the 6.5 m MMT in the z' and Y bands allow the detection of potential cluster members via photometric r…

2009 The Astrophysical Journal
eHST 6
Variable Intrinsic Absorption in Mrk 279
DOI: 10.1088/0004-637X/694/1/438 Bibcode: 2009ApJ...694..438S

Scott, Jennifer E.; Kriss, Gerard A.; Quijano, Jessica Kim +5 more

We examine the variability in the intrinsic absorption in the Seyfert 1 galaxy Mrk 279 using three epochs of observations from the Far Ultraviolet Spectroscopic Explorer and two epochs of observations with the Space Telescope Imaging Spectrograph on the Hubble Space Telescope. Rather than finding simple photoionization responses of the absorbing g…

2009 The Astrophysical Journal
eHST 5
A Statistical Study of the Relationship Between the Transport Rate of Magnetic Helicity and Solar Flares
DOI: 10.1088/0004-637X/704/2/1622 Bibcode: 2009ApJ...704.1622Z

Tan, Baolin; Zhang, Yin; Yan, Yihua

We present a statistical study which is aimed at understanding the fact that some flares (type I flare) are associated with sharp variations of the transport rate of magnetic helicity (dH/dt) while others are not (type II flare). The sample consists of 49 M-class and X-class flares which were produced by nine isolated active regions. Using high te…

2009 The Astrophysical Journal
SOHO 5
Evolutionary Status of 85 Pegasi
DOI: 10.1088/0004-637X/703/1/362 Bibcode: 2009ApJ...703..362B

Lee, J.; Demarque, P.; Kim, Y. -C. +1 more

We have investigated the evolutionary status of the visual binary 85 Peg (HD 224930) using a high-resolution spectroscopic analysis and the astrometric calibration of the stellar parameters. In spite of well-determined stellar parameters from HIPPARCOS astrometry and from spectroscopy, 85 Peg has for a long time revealed peculiar properties when a…

2009 The Astrophysical Journal
Hipparcos 5
Deconstructing Active Region AR10961 Using STEREO, Hinode, TRACE, and SOHO
DOI: 10.1088/0004-637X/703/2/1923 Bibcode: 2009ApJ...703.1923N

Walsh, Robert W.; Marsh, M. S.; Noglik, Jane B. +1 more

Active region 10961 was observed over a five-day period (2007 July 2-6) by instrumentation on-board STEREO, Hinode, TRACE, and SOHO. As it progressed from Sun's center to the solar limb, a comprehensive analysis of the extreme ultraviolet, X-ray, and magnetic field data reveals clearly observable changes in the global nature of the region. Tempera…

2009 The Astrophysical Journal
Hinode SOHO 5
Dynamics of Lyman Break Galaxies and Their Host Halos
DOI: 10.1088/0004-637X/703/1/198 Bibcode: 2009ApJ...703..198L

Koo, David C.; Lowenthal, James D.; Simard, Luc +1 more

We present deep two-dimensional spectra of 22 candidate and confirmed Lyman break galaxies (LBGs) at redshifts 2 < z < 4 in the Hubble Deep Field (HDF) obtained at the Keck II telescope. The targets were preferentially selected with spatial extent and/or multiple knot morphologies, and we used slitmasks and individual slits tilted to optimiz…

2009 The Astrophysical Journal
eHST 5
Coronal Radiation Belts
DOI: 10.1088/0004-637X/698/2/L86 Bibcode: 2009ApJ...698L..86H

Hudson, H. S.; MacKinnon, A. L.; De Rosa, M. L. +1 more

The magnetic field of the solar corona has a large-scale dipole character, which maps into the bipolar field in the solar wind. Using standard representations of the coronal field, we show that high-energy ions can be trapped stably in these large-scale closed fields. The drift shells that describe the conservation of the third adiabatic invariant…

2009 The Astrophysical Journal
SOHO 5
A Chandra X-ray Observation of L1251B
DOI: 10.1088/0004-637X/694/1/425 Bibcode: 2009ApJ...694..425S

Simon, Theodore

I report the results of a 60 ks X-ray observation of the L1251 dark cloud in Cepheus, which was acquired with the ACIS-I camera on board the Chandra X-Ray Observatory. Forty-three compact X-ray sources were detected. The field of view was centered on the position of IRAS 22376+7455, an embedded Class 0/I protostar that is closely associated with t…

2009 The Astrophysical Journal
XMM-Newton 4
UV Transient Brightenings Associated with a Coronal Mass Ejection
DOI: 10.1088/0004-637X/697/1/L72 Bibcode: 2009ApJ...697L..72S

Romoli, M.; Poletto, G.; Schettino, G.

In this paper, we analyze transient UV brightenings in spectra acquired by SOHO/UltraViolet Coronagraph Spectrometer (UVCS) on 2003 June 2 in association with a coronal mass ejection (CME) that occurred at the West limb of the Sun at 08:54 UT. Brightenings have been observed in lines from cool (C III, O VI), intermediate (Si VIII, Si XII), and hig…

2009 The Astrophysical Journal
SOHO 4