papers

Publications (31)

astro-ph.HE2010

The Super-Soft X-ray Phase of Nova RS Ophiuchi 2006

J. P. Osborne, K. L. Page, A. P. Beardmore +13

Swift X-ray observations of the ~60 day super-soft phase of the recurrent nova RS Ophiuchi 2006 show the progress of nuclear burning on the white dwarf in exquisite detail. First s…

astro-ph2001

Search for low-mass PMS companions around X-ray selected late B stars

S. Hubrig, D. Le Mignant, P. North +1

We have observed 49 X-ray detected bright late B-type dwarfs to search for close low-mass pre-main sequence (PMS) companions using the European Southern Observatory's ADONIS (Adapt…

astro-ph1997

Identification of selected sources from the ROSAT Galactic Plane Survey - I

C. Motch, P. Guillout, F. Haberl +6

We report on optical searches in the error circles of 93 ROSAT survey sources located at low galactic latitudes (|b| < 20 deg). These sources were extracted from the ROSAT Galactic…

astro-ph2004

Identification of a complete sample of northern ROSAT All-Sky Survey X-ray sources. VIII. The late-type stellar component

F. -J. Zickgraf, J. Krautter, S. Reffert +4

We present results of an investigation of the X-ray properties, age distribution, and kinematical characteristics of a high-galactic latitude sample of late-type field stars select…

astro-ph2008

Swift Observations of Shock Evolution in RS Ophiuchi

M. F. Bode, J. P. Osborne, K. L. Page +11

Our \textit{Swift} observations of RS Oph form an unprecedented X-ray dataset to undertake investigations of both the central source and the interaction of the outburst ejecta with…

astro-ph.SR2016

Pan-Chromatic observations of the Recurrent Nova LMC 2009a (LMC 1971b)

M. F. Bode, M. J. Darnley, A. P. Beardmore +11

Nova LMC 2009a is confirmed as a Recurrent Nova (RN) from positional coincidence with nova LMC 1971b. The observational data set is one of the most comprehensive for any Galactic o…

astro-ph2006

Infrared observations of the 2006 outburst of the recurrent nova RS Ophiuchi: the early phase

A. Evans, T. Kerr, Bin Yang +20

We present infrared spectroscopy of the recurrent nova RS Ophiuchi, obtained 11.81, 20.75 and 55.71 days following its 2006 eruption. The spectra are dominated by hydrogen recombin…

astro-ph2000

Identification of a complete sample of northern ROSAT All-sky survey X-ray sources. VII. The AGN subsample

I. Appenzeller, F. -J. Zickgraf, J. Krautter +1

In order to derive statistical properties of a complete X-ray selected sample of AGN we used the classification spectra of the RASS Selected Areas-North survey to study the luminos…

astro-ph1998

A New Cataclysmic Variable RX J0757.0+6306: Candidate for the Shortest Period Intermediate Polar

G. H. Tovmassian, J. Greiner, P. Kroll +8

A new cataclysmic variable is identified as the optical counterpart of the faint and hard X-ray source RX J0757.0+6306 discovered during the ROSAT all-sky survey. Strong double-pea…

astro-ph2006

The Spitzer IRS view of V4334 Sgr (Sakurai's Object)

A. Evans, V. H. Tyne, J. Th. van Loon +11

We present an observation of the very late thermal pulse object V4334 Sgr (Sakurai's Object) with the Infrared Spectrometer (IRS) on the Spitzer Space Telescope. The emission from…

astro-ph.SR2010

The peculiar dust shell of Nova DZ Cru (2003)

A. Evans, R. D. Gehrz, C. E. Woodward +10

We present Spitzer Space Telescope observations of the "peculiar variable" DZ Cru, identified by Rushton et al. (2008, MNRAS, 386, 289) as a classical nova. A dust shell, on which…

astro-ph.SR2012

Infrared observations of the recurrent nova T Pyxidis: ancient dust basks in the warm glow of the 2011 outburst

A. Evans, R. D. Gehrz, L. A. Helton +15

We present Spitzer Space Telescope and Herschel Space Observatory infrared observations of the recurrent nova T Pyx during its 2011 eruption, complemented by ground-base optical-in…

astro-ph2003

The Early Ultraviolet Evolution of the ONeMg Nova V382 Velorum 1999

S. N. Shore, G. Schwarz, H. E. Bond +7

We present a multiwavelength study of the ONeMg Galactic nova V382 Velorum 1999 using HST/STIS and FUSE ultraviolet spectra and comparisons with published groundbased optical spect…

astro-ph2001

The New AM Her System RX J0704.2+6203. Northern Twin of BL Hyi

G. H. Tovmassian, P. Szkody, J. Greiner +6

We report here on the identification and study of the optical counterpart of the ROSAT source RX J0704.2+6203. Extensive spectral and photometric observation showed that the object…

astro-ph2007

Silicate dust in the environment of RS Ophiuchi following the 2006 eruption

A. Evans, C. E. Woodward, L. A. Helton +20

We present further Spitzer Space Telescope observations of the recurrent nova RS Ophiuchi, obtained over the period 208-430 days after the 2006 eruption. The later Spitzer IRS data…

astro-ph2004

Late-type field stars in the RASS at high galactic latitude

F. -J. Zickgraf, J. Krautter, S. Frink +4

We present results of an investigation on a high-galactic latitude sample of late-type field stars selected from the ROSAT All-Sky Survey (RASS). The sample comprises about 200 G,…

astro-ph1997

RX J0719.2+6557: A new eclipsing polar

G. H. Tovmassian, J. Greiner, F. -J. Zickgraf +5

A new magnetic cataclysmic variable is identified as the counterpart of the X-ray source RX J0719.2+6557. The emission lines show radial velocity variations with a period of 98.2 m…

astro-ph1999

The late-type stellar component in the ROSAT All-Sky Survey at high galactic latitude

F. -J. Zickgraf, J. M. Alcala, E. Covino +4

We investigated the properties of the late-type stellar component in the RASS at high-galactic latitude |b| based on an optically identified sample of ROSAT All-Sky Survey (RASS) X…

astro-ph2001

The Reanalysis of the ROSAT Data of GQ Mus (1983) Using White Dwarf Atmosphere Emission Models

S. Balman, J. Krautter

The analyses of X-ray emission from classical novae during the outburst stage have shown that the soft X-ray emission below 1 keV, which is thought to originate from the photospher…

astro-ph1999

Identification of a complete sample of northern ROSAT All-Sky Survey X-ray sources. IV. Statistical analysis

J. Krautter, F. -J. Zickgraf, I. Appenzeller +8

We present the statistical evaluation of a count rate and area limited complete sample of the ROSAT All-Sky Survey (RASS) comprising 674 sources. The RASS sources are located in si…

astro-ph.SR2016

Rise and fall of the dust shell of the classical nova V339 Delphini

A. Evans, D. P. K. Banerjee, R. D. Gehrz +16

We present infrared spectroscopy of the classical nova V339 Delphini, obtained over a year period. The infrared emission lines were initially symmetrical, with HWHM velocit…

astro-ph.SR2020

The infrared view of dust and molecules around V4334 Sgr (Sakurai's Object): a 20-year retrospective

A. Evans, R. D. Gehrz, C. E. Woodward +16

We present an analysis of the evolution of circumstellar dust and molecules in the environment of the very late thermal pulse object V4334 Sgr (Sakurai's Object) over a -ye…

astro-ph1996

RX J0719.2+6557: A New Eclipsing Polar

G. Tovmassian, J. Greiner, F. -J. Zickgraf +4

A new magnetic, eclipsing cataclysmic variable is identified as the counterpart of the X-ray source RX J0719.2+6557 detected during the ROSAT all-sky survey. The relative phasing o…

astro-ph2000

The ORFEUS II Echelle Spectrometer: Instrument description, performance and data reduction

J. Barnstedt, N. Kappelmann, I. Appenzeller +11

During the second flight of the ORFEUS-SPAS mission in November/December 1996, the Echelle spectrometer was used extensively by the Principal and Guest Investigator teams as one of…

astro-ph.SR2011

Solid-phase C_60 in the peculiar binary XX Oph?

A. Evans, J. Th. van Loon, C. E. Woodward +8

We present infrared spectra of the binary XX Oph obtained with the Infrared Spectrograph on the Spitzer Space Telescope. The data show some evidence for the presence of solid C_60…

astro-ph.HE2011

XMM-Newton X-ray and UV observations of the fast nova V2491 Cyg during the supersoft source phase

J. -U. Ness, J. P. Osborne, A. Dobrotka +12

Two XMM observations of the fast classical nova V2491Cyg were carried out on days 39.93 and 49.62 after discovery, during the supersoft source (SSS) phase, yielding simultaneous X-…

astro-ph2005

An X-ray emission line spectrum of Nova V382 Velorum 1999

J. -U. Ness, S. Starrfield, C. Jordan +2

We report on the analysis of an X-ray grating spectrum of the Classical Nova V382 Vel (1999), obtained with the LETG+HRC-S instrument on board CHANDRA, which shows emission lines d…

astro-ph2007

Spitzer and ground-based infrared observations of the 2006 eruption of RS Ophiuchi

A. Evans, C. E. Woodward, L. A. Helton +18

We present Spitzer Space Telescope and complementary ground-based infrared observations of the recurrent nova RS Ophiuchi, obtained over the period 64-111 days after the 2006 erupt…

astro-ph2007

The SSS phase of RS Ophiuchi observed with Chandra and XMM-Newton I.: Data and preliminary Modeling

J. -U. Ness, S. Starrfield, A. P. Beardmore +13

The phase of Super-Soft-Source (SSS) emission of the sixth recorded outburst of the recurrent nova RS Oph was observed twice with Chandra and once with XMM-Newton. The observations…

astro-ph2006

Swift observations of the 2006 outburst of the recurrent nova RS Ophiuchi: I. Early X-ray emission from the shocked ejecta and red giant wind

M. F. Bode, T. J. O'Brien, J. P. Osborne +16

RS Ophiuchi began its latest outburst on 2006 February 12. Previous outbursts have indicated that high velocity ejecta interact with a pre-existing red giant wind, setting up shock…

astro-ph2003

A Chandra LETGS observation of V4743 Sagittarius: A Super Soft X-ray Source and a Violently Variable Light Curve

J. -U. Ness, S. Starrfield, V. Burwitz +13

V4743 Sgr (Nova Sgr 2002 No. 3) was discovered on 20 September 2002. We obtained a 5ks ACIS-S spectrum in November 2002 and found that the nova was faint in X-rays. We then obtaine…