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M. Spera

43 papers hereh-index 5520.2k citations165 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author5
  • middle author18
  • last author14

Across the 37 of 43 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA20
  • astro-ph.HE13
  • astro-ph.SR6
  • gr-qc2
  • astro-ph.CO1
  • astro-ph.EP1
same name
  • M. Spera — 3 papers
  • M. Spera — 2 papers
  • M. Spera — 2 papers

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20132021
most citedVery massive stars, pair-instability supernovae and intermediate-mass black holes with the SEVN code

344 citations · 1.8k across the 21 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.GA2016

Dynamics of supernova remnants in the Galactic Centre

Elisa Bortolas, Michela Mapelli, Mario Spera

The Galactic centre (GC) is a unique place to study the extreme dynamical processes occurring near a super-massive black hole (SMBH). Here we simulate a large set of binaries orbit…

astro-ph.GA2016

Brownian motion of massive black hole binaries and the final parsec problem

E. Bortolas, A. Gualandris, M. Dotti +2

Massive black hole binaries (BHBs) are expected to be one of the most powerful sources of gravitational waves (GWs) in the frequency range of the pulsar timing array and of forthco…

astro-ph.SR2016

Shedding light on the black hole mass spectrum

Mario Spera, Nicola Giacobbo, Michela Mapelli

The mass spectrum of stellar black holes (BHs) is highly uncertain. Theoretical models of BH formation strongly depend on the efficiency of stellar winds of the progenitor star and…

astro-ph.SR2016

Do open star clusters evolve toward energy equipartition?

Mario Spera, Michela Mapelli, Robin D. Jeffries

We investigate whether open clusters (OCs) tend to energy equipartition, by means of direct N-body simulations with a broken power-law mass function. We find that the simulated OCs…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.