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RR Lyrae stars in the Large Magellanic Cloud as seen by Gaia

Left panels: G-band light curves of RR Lyrae stars in the Large Magellanic Cloud observed by Gaia during the EPSL scanning. Right panels: I-band light curves obtained for the same stars by the OGLE IV...

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Call for observing proposals at the 1.52m Cassini Telescope

Proposals may be submitted for the August 1st, 2015 – January 31st, 2016 semester. The deadline is June 19th, 2015, at 13:00 UT.…

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OABO news from Gaia

A press release by G. Clementini (INAF-OABO), V. Ripepi (INAF-OACN), S. Leccia (INAF-OACN), et al. was published yesterday (May 28, 2015) on the ESA Gaia web page showing results from the DPAC-CU7...

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V404 Cygni outburst observed at Loiano

The X-ray binary V404 Cygni underwent an outburst detected in the X-ray band by Swift on June 18, 2015. One of the components of this source is a black hole weighing about 10 solar masses, and it is...

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MAORY KICK OFF MEETING

Image taken at the MAORY kick-off meeting in Bologna. A new era for the Adaptive Optics. MAORY the Multi Conjugate Adaptive Optics RelaY for E-ELT entered in a new era. After the agreement signed on...

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Giornate di Osservatorio

18 e 19 Febbraio 2016 Giornate di Osservatorio – Programma

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DDO68

DDO 68 , una pulce di Galassia ma vorace Un team internazionale di ricercatori guidato da Francesca Annibali, Cassini Fellowship presso l’Osservatorio Astronomico di Bologna dell’Istituto Nazionale di...

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Gaia Data Release 1

The Gaia spacecraft was launched on December 19th, 2013 to perform a 5-year long all-sky scanning survey that will provide exquisitely accurate astrometry (100 times better than Hipparcos) and...

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Gaia16aye: the first binary microlensing event ever discovered towards the...

On 2016-08-05 the 1.2 mag brightening of an otherwise quiet stellar source triggered the Gaia16aye Gaia Science Alert, nicknamed Ayers Rock (19:40:01.13 +30:07:53.4, J2000). The previous 22 Gaia...

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SECCO 1: a very dark stellar system lost in Virgo

Left panel: Hα images of the two bodies of SECCO 1 (projected separation ~6 kpc ) extracted from the MUSE data cube. Right panels: HST -ACS images of the same region.  At the distance of  the object 10...

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