activity
20212024
most citedDetection of He++ ion in the star-forming ring of the Cartwheel using MUSE data and ionizing mechanisms

21 citations · 61 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2024

X-Shooting ULLYSES: Massive stars at low metallicity VII. Stellar and wind properties of B supergiants in the Small Magellanic Cloud

M. Bernini-Peron, A. A. C. Sander, V. Ramachandran +22

Context. B supergiants (BSGs) represent an important connection between the main sequence and more extreme evolutionary stages of massive stars. Additionally, lying toward the cool…

astro-ph.GA2024

Chemical abundances and ionizing mechanisms in the star-forming double-ring of AM 0644-741 using MUSE data

V. M. A. Gómez-González, Y. D. Mayya, J. Zaragoza-Cardiel +6

We present the analysis of archival Very Large Telescope (VLT) Multi-Unit Spectroscopic Explorer (MUSE) observations of 179 HII regions in the star-forming double-ring collisional…

astro-ph.GA2024

Ages and metallicities of globular clusters in M81 using GTC/OSIRIS spectra

Luis Lomelí-Núñez, Y. D. Mayya, L. H. Rodríguez-Merino +8

We here present the results of an analysis of the optical spectroscopy of 42 globular cluster (GC) candidates in the nearby spiral galaxy M81 (3.61~Mpc). The spectra were obtained…

astro-ph.GA20234 cited

Star formation history of the post-collisional Cartwheel galaxy using Astrosat/UVIT FUV images

Y. D. Mayya, Sudhanshu Barway, V. M. A. Gómez-González +1

We present the results obtained by analysing new Astrosat/UVIT far ultraviolet (FUV) image of the collisional-ring galaxy Cartwheel. The FUV emission is principally associated with…

astro-ph.SR202314 cited

Spectroscopic and evolutionary analyses of the binary system AzV 14 outline paths toward the WR stage at low metallicity

D. Pauli, L. M. Oskinova, W. -R. Hamann +16

The origin of the observed population of Wolf-Rayet (WR) stars in low-metallicity (low-Z) galaxies, such as the Small Magellanic Cloud (SMC), is not yet understood. Standard, singl…

astro-ph.GA202316 cited

The stellar population responsible for a kiloparsec size superbubble seen in the JWST "phantom" images of NGC628

Y. D. Mayya, J. A. Alzate, L. Lomelí-Núñez +11

We here study the multi-band properties of a kiloparsec-size superbubble in the late-type spiral galaxy NGC628. The superbubble is the largest of many holes seen in the early relea…