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D. Bhattacharyya

4 papers hereh-index 26 citations9 works total

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

author position
  • first author4

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE1
same name
  • D. Bhattacharyya — 11 papers, h 38
  • D. Bhattacharyya — 9 papers, h 40
  • D. Bhattacharyya — 5 papers, h 25
  • D. Bhattacharyya — 4 papers, h 4
  • D. Bhattacharyya — 3 papers, h 2
  • D. Bhattacharyya — 3 papers, h 7

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
20172023
most citedCosmic spin and mass evolution of black holes and its impact

3 citations · 5 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2023★ 1 cited

Where can we find the merger remnant in BH-BH mergers in Globular clusters?

Dipanweeta Bhattacharyya, Jasjeet Singh Bagla

Mergers of black holes and other compact objects produce gravitational waves which carry a part of the energy, momentum, and angular momentum of the system. Due to asymmetry in the…

astro-ph.HE2020★ 3 cited

Cosmic spin and mass evolution of black holes and its impact

Dipanweeta Bhattacharyya, A. Mangalam

We build an evolution model of the central black hole that depends on the processes of gas accretion, the capture of stars, mergers as well as electromagnetic torque. In case of ga…

astro-ph.GA2018

Evolution of the M∙​−σ relation

D. Bhattacharyya, A. Mangalam

Black holes at the centers of the galaxies grow mainly by the processes of accretion, mergers, and consumption of stars. In the case of gas accretion with cooling sources, the flow…

astro-ph.GA2017★ 1 cited

The M∙​−σ relation in spherical systems

Dipanweeta Bhattacharyya, A. Mangalam

To investigate the M∙​−σ relation, we consider realistic elliptical galaxy profiles that are taken to follow a single power law density profile given by $ρ(r) = ρ_{0}(r/ r…

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