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On July 1st 2025 the third interstellar object, 3I/ATLAS or C/2025 N1 (ATLAS), was discovered, with an eccentricity of $e=6.15 \pm 0.01$ and perihelion of $q=1.357\pm0.001$ au. We report our initial visible to near-infrared (420-1000 nm)…

The discovery of deep spectral features in the X-ray spectrum of 1E1207.4-5209 focussed the attention of the astronomical community on this radio-quiet NS, making it the most intensively observed INS ever. The harvest of X-ray photons,…

天体物理学 · 物理学 2007-05-23 G. F. Bignami , A. De Luca , P. A. Caraveo , S. Mereghetti , M. Moroni , R. P. Mignani

We have made the first detection of a near-infrared counterpart associated with the disk around Radio Source "I," a massive protostar in the Kleinmann-Low Nebula in Orion using imaging with laser guide star adaptive optics on the Keck II…

3C318, a radio-loud quasar at z=1.574, is a subgalactic-sized radio source, and a good test-bed for the interplay between black hole and galaxy growth in the high-z Universe. Based on its IRAS, ISO, and SCUBA detections, it has long been…

星系天体物理 · 物理学 2016-01-13 P. Podigachoski , P. D. Barthel , R. F. Peletier , S. Steendam

The results of the photometric observations of comet C/2009 P1 (Garradd) performed at the 60-cm Zeiss-600 telescope of the Terskol observatory have been analyzed. During the observations, the comet was at the heliocentric and geocentric…

地球与行星天体物理 · 物理学 2021-01-15 A. V. Ivanova , S. A. Borisenko , M. V. Andreev

We present a new analysis of ${\it Spitzer}$ observations of comet 29P/Schwassmann-Wachmann 1 taken on UT 2003 November 21, 23, and 24, similar to a previous investigation of the observations (Stansberry et al. 2004), but using the most…

地球与行星天体物理 · 物理学 2015-08-06 Charles A. Schambeau , Yanga R. Fernandez , Carey M. Lisse , Nalin Samarasinha , Laura M. Woodney

We present LOFAR observations of one of the most spectacular objects in the radio sky: Abell 2255. This is a nearby ($z = 0.0806$) merging galaxy cluster hosting one of the first radio halos ever detected in the intra-cluster medium (ICM).…

We observed the large and faint planetary nebula (PN) around IN Com in H-alpha and [NII] light with a coronagraphic CCD device on the Wise Observatory reflector blocking the light from the central star. Our goal was to provide a second…

天体物理学 · 物理学 2009-10-31 Noah Brosch , Yehuda Hoffman

Comet Hale-Bopp was observed five times with ISOPHOT, the photometer on board the Infrared Space Observatory (ISO). Each time broadband photometry was performed using 4 different detectors, 5 apertures and, 10 filters covering the range…

The X-ray observatories XMM-Newton and Chandra provided a wealth of exciting new results. Chandra delivered X-ray images of outstanding detail, reaching subarcsecond spatial resolution for the first time in X-ray astronomy. XMM-Newton…

天体物理学 · 物理学 2007-05-23 Stefanie Komossa

We report the discovery of the first hyperluminous infrared galaxy (HyLIG) in the course of the European Large Area ISO Survey (ELAIS). This object has been detected by ISO at 6.7, 15, and 90 microns, and is found to be a broad-line,…

We report the discovery of a new bright quasar PHL 1811 as part of a followup program to identify bright quasars in the FIRST radio survey. With B=13.9, R=13.9, and z=0.192, this quasar is now the second brightest quasar (in apparent…

天体物理学 · 物理学 2009-11-06 K. M. Leighly , J. P. Halpern , D. J. Helfand , R. H. Becker , C. D. Impey

We report the first detection of flux variability in the most luminous X-ray source in the southern ring of the Cartwheel galaxy. XMM--Newton data show that the luminosity has varied over a timescale of six months from L[0.5-10] keV \~1.3…

天体物理学 · 物理学 2009-11-11 A. Wolter , G. Trinchieri , M. Colpi

The Infrared Space Observatory (ISO) was an extremely successful european space mission that gave us an unparallel view of the Universe in the infrared, and provided us with hundreds of observations of star forming regions and bipolar…

天体物理学 · 物理学 2007-05-23 Alberto Noriega-Crespo

The coherence of the interaction of light with a collisionless gas (Einstein 1917) founds the theory of gas lasers. It is, for the understanding of universe, a simpler and more powerful tool than the big bang which requires questionable…

综合物理 · 物理学 2015-06-15 Jacques Moret-Bailly

Since its launch in 1990, the Hubble Space Telescope (HST) has served as a platform with unique capabilities for remote observations of comets in the far-ultraviolet region of the spectrum. Successive generations of imagers and…

地球与行星天体物理 · 物理学 2018-04-24 Paul D. Feldman , Harold A. Weaver , Michael F. A'Hearn , Michael R. Combi , Neil Dello Russo

Eleven years after its perihelion, comet C/1995 O1 (Hale-Bopp) is still active. Between October 20--22, 2007, we detected a diffuse coma of 180x10^3$km in diameter with a slight elongation toward N/S direction. The integrated brightness was…

天体物理学 · 物理学 2009-11-13 Gy. M. Szabo , L. L. Kiss , K. Sarneczky

NASA's Chandra X-ray Observatory and ESA's XMM-Newton made their first observations one decade ago. The unprecedented and complementary capabilities of these observatories to detect, image, and measure the energy of cosmic X-rays, achieved…

高能天体物理现象 · 物理学 2015-07-15 Maria Santos-Lleo , Norbert Schartel , Harvey Tananbaum , Wallace Tucker , Martin C. Weisskopf

Comet Hale--Bopp (C/1995 O1) has been the single most significant comet encountered by modern astronomy, still having displayed significant activity at 25.7 AU solar distance in late 2007. It is a puzzling question when and where this…

地球与行星天体物理 · 物理学 2015-05-27 Gy. M. Szabó , K. Sárneczky , L. L. Kiss

The SPIREX telescope, located at the Amundsen-Scott South Pole Station, was a prototype system developed to exploit the excellent conditions for IR observing at the South Pole. Observations over two winter seasons achieved remarkably deep,…

天体物理学 · 物理学 2007-05-23 J. M. Rathborne , M. G. Burton