Catalog of supersoft X-ray sources

Abstract

This catalog comprises an up-to-date (December 1999) list of luminous (>10^36 erg/s), binary supersoft X-ray sources. This electronic version (including the accompannying Web-pages) supersedes the printed version of Greiner (1996).

publ. in New Astr. 5, 137; full electronic version of the catalog at http://www.aip.de/People/JGreiner/sss/ssscat.html

Cited by in corpus (72)

• Constraints on the Progenitor System of the Type Ia Supernova SN 2011fe/PTF11kly
• Thermal Stability of White Dwarfs Accreting Hydrogen-rich Matter and Progenitors of Type Ia Supernovae
• The COS-Halos Survey: Origins of the Highly Ionized Circumgalactic Medium of Star-Forming Galaxies
• The Progenitors of Type Ia Supernovae: Are They Supersoft Sources?
• Luminous Supersoft X-Ray Sources in External Galaxies
• The first binary star evolution model producing a Chandrasekhar mass white dwarf
• The central region of M31 observed with XMM-Newton. II. Variability of the individual sources
• Chandra Discovery of Luminous Supersoft X-Ray Sources in M81
• XMM-Newton survey of the Local Group galaxy M 33
• A Chandra observation of the interacting pair of galaxies NGC 4485/NGC 4490
• XMM-Newton survey of M 31
• Supersoft X-ray Sources in M31: I. A Chandra Survey and an Extension to Quasisoft Sources
• Discovery of an Ultrasoft X-ray Transient Source in the 2XMM Catalog: a Tidal Disruption Event Candidate
• Surface Hydrogen Modeling of Super Soft X-ray Sources: Are They Supernova Ia Progenitors?
• Effects of rotation on the helium burning shell source in accreting white dwarfs
• The Progenitors of Type Ia Supernovae: II. Are they Double-Degenerate Binaries? The Symbiotic Channel
• The Discovery of Quasisoft and Supersoft Sources in External Galaxies
• An Ultrasoft X-ray Flare from 3XMM J152130.7+074916: a Tidal Disruption Event Candidate
• Revisiting the ultraluminous supersoft source in M101: an optically thick outflow model
• A Luminous Recurrent Supersoft X-ray Source in NGC 300
• A Luminous Be+White Dwarf Supersoft Source in the Wing of the SMC: MAXI J0158-744
• X-ray Point Sources in the Sombrero Galaxy: Supersoft sources, the globular cluster/LMXB connection, and an overview
• SPH simulations of irradiation-driven warped accretion discs and the long periods in X-ray binaries
• A Close Look at the Population of Supersoft and Quasi-Soft X-Ray Sources Observed in M31 with XMM-Newton
• An XMM-Newton view of M101: I. The luminous X-ray source population
• No hot and luminous progenitor for Tycho's supernova
• Supersoft X-ray Sources. Parameters of Stellar Atmospheres
• The planetary nebula Abell 48 and its [WN] nucleus
• The first pre-supersoft X-ray binary
• The Sources of Extreme Ultraviolet and Soft X-ray Backgrounds
• An XMM-Newton view of M101 - II. Global X-ray source properties
• Upper limits on bolometric luminosities of ten type Ia supernova progenitors from Chandra observations
• Time variability of X-ray sources in the M 31 centre field
• Radio sources in the Chandra Galactic Bulge survey
• XMM-Newton discovery of 217 s pulsations in the brightest persistent supersoft X-ray source in M31
• Evidence for Optically Thick, Eddington-limited Winds Driven by Supercritical Accretion
• Rapidly accreting white dwarfs as supernova type Ia progenitors
• Limits on the X-ray and optical luminosity of the progenitor of the type Ia supernova SN2007sr
• Supersoft X-ray sources in M31: II. ROSAT-detected supersoft sources in the ROSAT, Chandra and XMM eras
• BZ Cam during its 1999/2000 optical low state
• The Short Period Supersoft Source in M31
• Discovery of the Candidate Off-nuclear Ultrasoft Hyper-luminous X-ray Source 3XMM J141711.1+522541
• Excluding super-soft X-ray sources as progenitors for four Type Ia supernovae in the Large Magellanic Cloud
• Obscuration of Supersoft X-ray Sources by Circumbinary Material - A Way to Hide Type Ia Supernova Progenitors?
• Balmer-Dominated Shocks Exclude Hot Progenitors for Many Type Ia Supernovae
• The X-ray properties of the dwarf Magellanic-type galaxy NGC 55
• Classification of X-ray Sources in the XMM-Newton Serendipitous Source Catalog: Objects of Special Interest
• X-ray source population study of the starburst galaxy M83 with XMM-Newton
• First optical identification of a suprsoft X-ray source in M31
• Soft band X/K luminosity ratios for gas-poor early-type galaxies
• The Recurrent Nova U Scorpii in the 1999 Outburst: the First Detection of a Significant Orbital-Period Change
• Progenitor constraints on the Type Ia supernova SN 2014J from Hubble Space Telescope H$\beta$ and [O III] observations
• A search for radio emission from Galactic supersoft X-ray sources
• Upper limits on bolometric luminosities of three type Ia supernova progenitors - New results in the ongoing Chandra archival search for type Ia supernova progenitors
• A helium-burning white dwarf binary as a supersoft X-ray source
• Accreting White Dwarfs as Supersoft X-ray Sources
• Transient Extremely Soft X-ray Emission from the Unusually Bright CV in the Globular Cluster M3: a New CV X-ray Luminosity Record?
• Detection of a Rare Supersoft Outburst Event during a Suzaku Observation of 1E0102.2-7219
• X-ray Limits on the Progenitor System of the Type Ia Supernova 2017ejb
• The Megasecond Chandra X-Ray Visionary Project Observation of NGC 3115 (II): properties of point sources
• Supersoft sources in M 31: Comparing the XMM-Newton Deep Survey, ROSAT and Chandra catalogues
• Supersoft X-Ray Nebulae in the Large Magellanic Cloud
• LIN 358: A symbiotic binary accreting above the steady hydrogen fusion limit
• Multiwavelength search for counterparts of supersoft X-ray sources in M31
• X Ray Observations of Classical and recurrent Novae in Outburst
• Revisiting multiwavelength data on the supersoft X-ray source CAL 83
• X-ray Development of the Classical Nova V2672 Ophiuchi with Suzaku
• Soft X-ray emission from the classical nova AT 2018bej
• The significant contribution of supersoft X-ray Sources to the nebular HeII line emission
• Examining the evolution of the Supersoft X-ray Source RX J0513.9-6951
• Transient X-ray Sources in the Magellanic-type Galaxy NGC 4449
• Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors