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We present multi-epoch infrared photometry and spectroscopy obtained with warm Spitzer, Subaru and SOFIA to assess variability for the young ($\sim$20 Myr) and dusty debris systems around HD 172555 and HD 113766A. No variations (within…

地球与行星天体物理 · 物理学 2020-07-29 Kate Y. L. Su , George H. Rieke , Carl Melis , Alan P. Jackson , Paul S. Smith , Huan Y. A. Meng , Andras Gaspar

We present an analysis of the gas-poor circumstellar material in the HD 113766 binary system (F3/F5, 10 - 16 Myr), recently observed by the Spitzer Space Telescope. For our study we have used the infrared mineralogical model derived from…

天体物理学 · 物理学 2009-11-13 C. M. Lisse , C. H. Chen , M. C. Wyatt , A. Morlok

Warm debris disks are a sub-sample of the large population of debris disks, and display excess emission in the mid-IR. Around solar-type stars, very few objects show emission features in mid-IR spectroscopic observations, that are…

We present high-resolution mid-infrared observations of the nearby late-type young binary system Hen 3-600. The binary, at a distance of $\sim$ 50 pc, could be a member of the TW Hydrae Association, the nearest known group of young stars,…

We review the X-ray observations of hot subdwarf stars. While no X-ray emission has been detected yet from binaries containing B-type subdwarfs, interesting results have been obtained in the case of the two luminous O-type subdwarfs HD…

高能天体物理现象 · 物理学 2015-06-11 Sandro Mereghetti , Nicola La Palombara , Paolo Esposito , Andrea Tiengo

Using the NASA/IRTF SpeX & BASS spectrometers we have obtained novel 0.7 - 13 um observations of the newly imaged HD36546 debris disk system. The SpeX spectrum is most consistent with the photospheric emission expected from an Lstar ~ 20…

太阳与恒星天体物理 · 物理学 2017-05-24 Carey M. Lisse , Mike L. Sitko , Ray W. Russell , Massimo Marengo , Thayne Currie , Carl Melis , Tushar Mittal , Inseok Song

We report an in-depth study of the F8-type star HD 166191, identified in an ongoing survey for stars exhibiting infrared emission above their expected photospheres in the Wide-field Infrared Survey Explorer all-sky catalog. The fractional…

太阳与恒星天体物理 · 物理学 2015-06-16 Adam Schneider , Inseok Song , Carl Melis , Ben Zuckerman , Mike Bessell , Tara Hufford , Sasha Hinkley

We aim at characterising the structure of the gas and dust around the high mass X-ray binary GX 301-2, a highly obscured X-ray binary hosting a hypergiant star and a neutron star, in order to better constrain its evolution. We used Herschel…

太阳与恒星天体物理 · 物理学 2015-06-23 Mathieu Servillat , Alexis Coleiro , Sylvain Chaty , Farid Rahoui , Juan Antonio Zurita Heras

We report the detection of dust emission at sub-millimeter wavelengths from HD 107146, a G2V star with an age estimated to lie between 80 and 200 Myr. The emission is resolved at 450um with a size 300 AU x 210 AU. A fit to the spectral…

We present analysis of both the resolved X-ray emission line profiles and the broadband X-ray spectrum of the O2 If* star HD 93129A, measured with the Chandra HETGS. This star is among the earliest and most massive stars in the Galaxy, and…

We report the discovery of four rare debris disks with warm excesses around F-stars, significantly increasing the number of such systems known in the solar neighborhood. Three of the disks are consistent with the predictions of steady state…

太阳与恒星天体物理 · 物理学 2009-08-05 A. Moór , D. Apai , I. Pascucci , P. Ábrahám , C. Grady , Th. Henning , A. Juhász , Cs. Kiss , Á. Kóspál

Using our previously reported observations, we derive some physical parameters of the moderately fast nova V2676 Ophiuchi 2012 # 1. The best-fit CLOUDY model of the nebular spectrum obtained on 2015 May 8 shows a hot white dwarf source with…

太阳与恒星天体物理 · 物理学 2019-04-10 Ashish Raj , M. Pavana , U. S. Kamath , G. C. Anupama , F. M. Walter

We present an X-ray binary population synthesis model, and use it to simulate the evolution of X-ray binaries formed in a burst of star formation of duration 20 Myr and star-formation rate 10 M_sun/yr. Our goal is to explain the hard (2-10…

天体物理学 · 物理学 2007-05-23 M. S. Sipior , M. Eracleous , S. Sigurdsson

We report resolution of a halo of X-ray line emission surrounding the Zero Age Main Sequence (ZAMS) G8.5V star HD 61005 by Chandra ACIS-S. Located only 36.4 pc distant, HD 61005 is young (approx. 100 Myr), x-ray bright (300 times Solar),…

We report on the discovery of X-ray emission from SN 1970G in M101, 35 years after its outburst, using deep X-ray imaging with the Chandra X-ray observatory. The Chandra ACIS spectrum shows that the emission is soft (<2 keV) and…

天体物理学 · 物理学 2009-11-11 Stefan Immler , K. D. Kuntz

We present a stacking analysis of 2.61 Msec of archival Chandra observations of stellar wind bow shocks. We place an upper limit on the X-ray luminosity of IR-detected bow shocks of $<2\times10^{29}$ erg s$^{-1}$, a more stringent…

高能天体物理现象 · 物理学 2019-04-24 Breanna A. Binder , Patrick Behr , Matthew S. Povich

A 90 ks Chandra HETG observation of the young stellar cluster NGC 6193 in the southern Ara OB1 association detected 43 X-ray sources in a 2' x 2' core region centered on the young O stars HD 150135 (O6.5V) and HD 150136 (O3+O6V). The…

天体物理学 · 物理学 2009-11-11 S. L. Skinner , S. A. Zhekov , F. Palla , C. L. D. R Barbosa

We present a spectral investigation of X-ray binaries in NGC 5128 (Cen A), using six 100 ks Chandra observations taken over two months in 2007. We divide our sample into thermally and non-thermally dominated states based on the behavior of…

The low resolution X-ray spectra around $\eta$ Car covering Tr 16 and part of Tr 14 have been extracted from a Chandra CCD ACIS image. Various analysis techniques have been applied to the spectra based on their count rates. The spectra with…

The nature of the mechanisms apparently driving X-rays from intermediate mass stars lacking strong convection zones or massive winds remains poorly understood, and the possible role of hidden, lower mass close companions is still unclear. A…

太阳与恒星天体物理 · 物理学 2015-06-19 Jeremy J. Drake , Jonathan Braithwaite , Vinay Kashyap , H. Moritz Guenther , Nicholas J. Wright
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