We report the first detection of the Galactic Center massive black hole, Sgr A*, at 100 μm and 160 μm. Our measurements were obtained with PACS on board the...
A detection of the donor star of Aquila X-1 during its 2004 outburst?
Phase-resolved high-resolution optical spectroscopy has revealed narrow NIII and HeII emission lines from the soft X-ray transient Aquila X-1 during its 2004...
A determination of the space density and birth rate of hydrogen-line (DA) white dwarfs in the Galactic plane, based on the UVEX survey
We present a determination of the average space density and birth rate of hydrogen-line (DA) white dwarfs within a radius of 1 kpc around the Sun, based on an...
A devil in the detail: parameter cross-talk from the solar cycle and estimation of solar p-mode frequencies
Frequencies, powers and damping rates of the solar p modes are all observed to vary over the 11-yr solar activity cycle. Here, we show that simultaneous...
A DIACHRONIC ANALYSIS OF ORIENTATION OF SACRED PRECINCTS ACROSS JORDAN
Located in the southern part of the Levant, the territory of present day Jordan functioned as a cultural crossroad since times immemorial. The state of...
A different approach to the cosmological quantized redshift problem
A new phenomenological model for the interpretation of the discrete redshift phenomenon is developed. The model, based on the basic physical notion of adiabatic...
A Differential Scanning Calorimetric (DSC) Study on Heavy Ozonized C60 Fullerene
The DSC (Differential Scanning Calorimetry) analysis of heavy ozonized C60 fullerene (known also as “fullerene ozopolymer”), shows the exothermal decomposition...
A diffuse tidal dwarf galaxy destined to fade out as a "dark galaxy"
We have explored the properties of a peculiar object detected in deep optical imaging and located at the tip of an H I tail emerging from Hickson Compact Group...
A Disintegrating Rocky Planet with Prominent Comet-like Tails around a Bright Star
We report the discovery of BD+05 4868 Ab, a transiting exoplanet orbiting a bright (V = 10.16) K-dwarf (TIC 466376085) with a period of 1.27 days. Observations...