Search Publications

The Chandra HRC View of the Subarcsecond Structures in the Nuclear Region of NGC 1068
DOI: 10.1088/0004-637X/756/2/180 Bibcode: 2012ApJ...756..180W

Elvis, Martin; Risaliti, Guido; Karovska, Margarita +2 more

We have obtained a high spatial resolution X-ray image of the nucleus of NGC 1068 using the High Resolution Camera (HRC-I) on board the Chandra X-ray Observatory, which provides an unprecedented view of the innermost 1 arcsec radius region of this galaxy. The HRC image resolves the narrow-line region into X-ray emission clumps matching bright emis…

2012 The Astrophysical Journal
eHST 23
Characteristic Size of Flare Kernels in the Visible and Near-infrared Continua
DOI: 10.1088/2041-8205/750/1/L7 Bibcode: 2012ApJ...750L...7X

Xu, Yan; Cao, Wenda; Jing, Ju +1 more

In this Letter, we present a new approach to estimate the formation height of visible and near-infrared emission of an X10 flare. The sizes of flare emission cores in three wavelengths are accurately measured during the peak of the flare. The source size is the largest in the G band at 4308 Å and shrinks toward longer wavelengths, namely the green…

2012 The Astrophysical Journal
SOHO 23
Properties of Umbral Dots from Stray Light Corrected Hinode Filtergrams
DOI: 10.1088/0004-637X/752/2/109 Bibcode: 2012ApJ...752..109L

Ichimoto, Kiyoshi; Ravindra, B.; Mathew, Shibu K. +3 more

High-resolution blue continuum filtergrams from Hinode are employed to study the umbral fine structure of a regular unipolar sunspot. The removal of scattered light from the images increases the rms contrast by a factor of 1.45 on average. Improvement in image contrast renders identification of short filamentary structures resembling penumbrae tha…

2012 The Astrophysical Journal
Hinode 23
A Suzaku Observation of Mkn 590 Reveals a Vanishing Soft Excess
DOI: 10.1088/0004-637X/759/1/63 Bibcode: 2012ApJ...759...63R

Rivers, Elizabeth; Markowitz, Alex; Rothschild, Richard +1 more

We have analyzed a long-look Suzaku observation of the Seyfert 1.2 Mkn 590. We aimed to measure the Compton reflection strength, Fe K complex properties, and soft excess emission as had been observed previously in this source. The Compton reflection strength was measured to be in the range 0.2-1.0 depending on the model used. A moderately strong F…

2012 The Astrophysical Journal
Suzaku XMM-Newton 23
Active Region Moss: Doppler Shifts from Hinode/Extreme-ultraviolet Imaging Spectrometer Observations
DOI: 10.1088/0004-637X/753/1/37 Bibcode: 2012ApJ...753...37T

Tripathi, Durgesh; Mason, Helen E.; Klimchuk, James A.

Studying the Doppler shifts and the temperature dependence of Doppler shifts in moss regions can help us understand the heating processes in the core of the active regions. In this paper, we have used an active region observation recorded by the Extreme-ultraviolet Imaging Spectrometer (EIS) on board Hinode on 2007 December 12 to measure the Doppl…

2012 The Astrophysical Journal
Hinode 23
First Science Results from SOFIA/FORCAST: The Mid-infrared View of the Compact H II Region W3A
DOI: 10.1088/2041-8205/749/2/L21 Bibcode: 2012ApJ...749L..21S

Schoenwald, J.; Zinnecker, H.; Tielens, A. G. G. M. +10 more

The massive star-forming region W3 was observed with the faint object infrared camera for the SOFIA telescope as part of the Short Science program. The 6.4, 6.6, 7.7, 19.7, 24.2, 31.5, and 37.1 µm bandpasses were used to observe the emission of polycyclic aromatic hydrocarbon (PAH) molecules, very small grains, and big grains. Optical depth …

2012 The Astrophysical Journal
ISO 23
Are Large, Cometary-shaped Proplyds Really (Free-floating) Evaporating Gas Globules?
DOI: 10.1088/2041-8205/761/2/L21 Bibcode: 2012ApJ...761L..21S

Sahai, R.; Morris, M. R.; Güsten, R.

We report the detection of strong and compact molecular line emission (in the CO J = 3-2, 4-3, 6-5, 7-6, 13CO J = 3-2, HCN, and HCO+ J = 4-3 transitions) from a cometary-shaped object (Carina-frEGG1) in the Carina star-forming region (SFR) previously classified as a photoevaporating protoplanetary disk (proplyd). We derive a …

2012 The Astrophysical Journal
eHST 23
Prospect of Studying Hard X- and Gamma-Rays from Type Ia Supernovae
DOI: 10.1088/0004-637X/760/1/54 Bibcode: 2012ApJ...760...54M

Yamaguchi, H.; Diehl, R.; Tamagawa, T. +9 more

We perform multi-dimensional, time-dependent radiation transfer simulations for hard X-ray and γ-ray emissions, following radioactive decays of 56Ni and 56Co, for two-dimensional delayed-detonation models of Type Ia supernovae (SNe Ia). The synthetic spectra and light curves are compared with the sensitivities of current and …

2012 The Astrophysical Journal
INTEGRAL 23
The Atacama Cosmology Telescope: High-resolution Sunyaev-Zel'dovich Array Observations of ACT SZE-selected Clusters from the Equatorial Strip
DOI: 10.1088/0004-637X/751/1/12 Bibcode: 2012ApJ...751...12R

Hilton, Matt; Hasselfield, Matthew; Sifón, Cristóbal +41 more

We present follow-up observations with the Sunyaev-Zel'dovich Array (SZA) of optically confirmed galaxy clusters found in the equatorial survey region of the Atacama Cosmology Telescope (ACT): ACT-CL J0022-0036, ACT-CL J2051+0057, and ACT-CL J2337+0016. ACT-CL J0022-0036 is a newly discovered, massive (sime 1015 M ), high-re…

2012 The Astrophysical Journal
Planck 23
A Direct Measurement of the Total Gas Column Density in Orion KL
DOI: 10.1088/0004-637X/744/1/28 Bibcode: 2012ApJ...744...28P

Comito, C.; Schilke, P.; Lis, D. C. +7 more

The large number of high-J lines of C18O available via the Herschel Space Observatory provide an unprecedented ability to model the total CO column density in hot cores. Using the emission from all the observed lines (up to J = 15-14), we sum the column densities in each individual level to obtain the total column after correcting for t…

2012 The Astrophysical Journal
Herschel 23