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TCP J18102829-2729590
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ATel 9658: Confirmation of TCP J18102829-2729590 in Sagittarius as a classical nova in the optically thick stage
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Blobrana
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IGR J17062-6143
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Title: X-ray emission and absorption features during an energetic thermonuclear X-ray burst from IGR J17062-6143 Authors: N. Degenaar, J. M. Miller, R. Wijnands, D. Altamirano, A. C. Fabian Type-I X-ray bursts are thermonuclear explosions occurring in the surface layers of accreting neutron...
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Gamma Sextantis
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Gamma Sextantis (8 Sextantis, HD 85558, HIP 48437, SAO 137199 and HR 3909) is a triple star system in the constellation Sextans. The triple star system comprises of a close binary pair of white dwarfs (stellar classification A1), and a more distant companion. The two Gamma Sextantis A and B componen...
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Blobrana
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PNV J00425145+4118352
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ATel 10098: UV/Optical discovery of a Possible Nova in M31
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Blobrana
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PTSS-17dmk
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ATel 10090: CNEOST OT PTSS-17dmk, discovery - new OT, no VIZIER data
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Blobrana
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BF Cygni
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ATel 7013: Large amplitude flare from symbiotic nova BF Cyg in outburst Position (2000): RA 19 23 53.5064 | Dec +29 40 29.220
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Blobrana
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CC Sculptoris
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Title: CC Sculptoris: Eclipsing SU UMa-Type Intermediate Polar Author: Taichi Kato (Kyoto U), Franz-Josef Hambsch (GEOS, BAV, VVS), Arto Oksanen (Nyrola Obs.), Peter Starr (Warrumbungle Obs.), Arne Henden (AAVSO) We observed the 2014 superoutburst of the SU UMa-type intermediate polar CC Sc...
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RZ Leonis
(Preview)
The dwarf nova RZ Leonis is in outburst. Date: 21st March, 2012 Magnitude: 11.5 - 19.2 V Period: - Satellite orbital period: 0.076038 days Spectral type: ? Position(2000): RA=11 37 22.27 | Dec=+01° 48' 58.5"
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NGC 2022
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NGC 2022 (also HD 37882, GC 1225, IRAS 05393+0903, PN G196.6-10.9, and PK 196-10 1) is a magnitude +12.8 planetary nebula located about 7,000 light-years away in the constellation Orion. Its central class O8V star is HD 37882 with a magnitude of +7.2 In an 8-inch telescope and dark skies it appears as...
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GRO J1744-28
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ATel 5810; Fermi/GBM Detection of 0.467s Pulsation from GRO J1744-28. The Bursting Pulsar (GRO J1744-28) is a low-mass x-ray binary with a period of 11.8 days. It was discovered in December 1995 by the Burst and Transient Source Experiment on the Compton Gamma-Ray Observatory Read more
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Blobrana
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PNV J16521887-3754189
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ATel 10071: PNV J16521887-3754189 is a New Galactic Nova in Scorpius
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USNO-A2.0 1200-1153830
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ATel 10070: USNO-A2.0 1200-1153830 is a binary star with a total eclipse with sharp transitions
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Blobrana
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IM Normae
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IM Normae (Nova Normae 1920) is a magnitude +18.5 eclipsing symbiotic-type recurrent nova located in the constellation Norma. The recurrent nova has only been seen in outburst on two occasions; as a magnitude +9.0 star recorded on a photographic plate exposed on the 6th July 1920 by I. E. Woods at Ha...
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Blobrana
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QSO B1142-225
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ATel 10068: MASTER: PKS 1142-225 optical flare
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WD 1425+540
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Hubble Witnesses Massive Comet-Like Object Pollute Atmosphere of a White Dwarf Astronomers have found the first evidence of the remains of a comet-like object scattered around a burned-out star. They used NASA's Hubble Space Telescope to detect the debris, which has polluted the atmosphere of a...
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