activity
20182022
most citedJINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe

51 citations · 124 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2024

The recent star formation histories of nearby galaxies on resolved scales

Maria Lomaeva, Amélie Saintonge, Ilse De Looze

Star formation histories (SFHs) of galaxies are affected by a variety of factors, both external (field vs. cluster/group) and internal (presence of a bar and AGN, morphological typ…

astro-ph.GA20226 cited

The recent star formation history of NGC 628 on resolved scales

Maria Lomaeva, Ilse De Looze, Amélie Saintonge +1

Star formation histories (SFHs) are integral to our understanding of galaxy evolution. We can study recent SFHs by comparing the star formation rate (SFR) calculated using differen…

astro-ph.HE202023 cited

High-resolution X-ray spectroscopy of the stellar wind in Vela X-1 during a flare

M. Lomaeva, V. Grinberg, M. Guainazzi +8

We present a 130 ks observation of the prototypical wind-accreting, high-mass X-ray binary Vela X-1 collected with XMM-Newton at orbital phases between 0.12 and 0.28. A stron…

astro-ph.GA202051 cited

JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe

I. De Looze, I. Lamperti, A. Saintonge +29

Scaling laws of dust, HI gas and metal mass with stellar mass, specific star formation rate and metallicity are crucial to our understanding of the buildup of galaxies through thei…

astro-ph.HE20195 cited

Vela X-1 as a laboratory for accretion in High-Mass X-ray Binaries

P. Kretschmar, S. Martínez-Núñez, F. Fürst +7

Vela X-1 is an eclipsing high mass X-ray binary (HMXB) consisting of a 283s accreting X-ray pulsar in a close orbit of 8.964 days around the B0.5Ib supergiant HD77581 at a distance…

astro-ph.GA201939 cited

Abundances of disk and Bulge giants from high-resolution optical spectra III. Sc, V, Cr, Mn, Co, Ni

M. Lomaeva, H. Jönsson, N. Ryde +2

Context. Recent observations of the Bulge, e.g., its X-shape, cylindrical stellar motions, and a potential fraction of young stars propose that it formed through secular evolution…