activity
20042024
most citedAn Ultraviolet-to-Radio Broadband Spectral Atlas of Nearby Galaxies

376 citations · 2.3k across the 30 of their papers we have counts for

collaborators

30 papers

astro-ph.SR2024★ 3 cited

Revealing the elusive companion of the red giant binary 2MASSJ05215658+4359220 from UV HST and Astrosat-UVIT data

Luciana Bianchi, John Hutchings, Ralph Bohlin +2

Black hole demographics in different environments is critical in view of recent results on massive-stars binarity, and of the multi-messenger detectability of compact objects merge…

astro-ph.SR2024★ 3 cited

Hot Stars in the GALEX Ultraviolet Sky Surveys (GUVcat_AISxSDSS_HS) and the Binary Fraction of Hot Evolved Stars

Luciana Bianchi

We present a catalog of 71,364 point-like UV sources with SDSS photometry and GALEX FUV-NUV less or equal 0.1mag. The limit corresponds to stellar Teff greater than 15,000 to 20,00…

astro-ph.GA2020★ 7 cited

New Results from the UVIT Survey of the Andromeda Galaxy

D. A. Leahy, J. Postma, M. Buick +3

The Andromeda Galaxy (M31) has been observed with the UltraViolet Imaging Telescope (UVIT) instrument onboard the AstroSat Observatory. The M31 sky area was covered with 19 fields,…

astro-ph.GA2020★ 7 cited

Dorado and its member galaxies. Ha imaging of the group backbone

R. Rampazzo, S. Ciroi, P. Mazzei +9

ABRIDGED: Dorado is a nearby, rich and clumpy galaxy group that extends for several degrees in the Southern Hemisphere. For the first time, we map the Ha distribution as a possible…

astro-ph.SR2020★ 9 cited

Chandra observations of the planetary nebula IC 4593

J. A. Toalá, M. A. Guerrero, L. Bianchi +2

The ACIS-S camera on board the Chandra X-ray Observatory has been used to discover a hot bubble in the planetary nebula (PN) IC4593, the most distant PN detected by Chandra so far.…

astro-ph.GA2018★ 6 cited

A multi-wavelength study of the evolution of Early-Type Galaxies in Groups: the ultraviolet view

R. Rampazzo, P. Mazzei, A. Marino +5

ABRIDGED- The UV-optical color magnitude diagram (CMD) of rich galaxy groups is characterised by a well developed Red Sequence (RS), a Blue Cloud (BC) and the so-called Green Valle…