---
_id: '17671'
abstract:
- lang: eng
  text: Galactic nuclei are expected to be densely populated with stellar and intermediate
    mass black holes. Exploring this population will have important consequences for
    the observation prospects of gravitational waves as well as understanding galactic
    evolution. The gas cloud G2 currently approaching Sgr A* provides an unprecedented
    opportunity to probe the black hole and neutron star population of the Galactic
    nucleus. We examine the possibility of a G2-black hole encounter and its detectability
    with current X-ray satellites, such as Chandra and NuSTAR. We find that multiple
    encounters are likely to occur close to the pericenter, which may be detectable
    upon favorable circumstances. This opportunity provides an additional, important
    science case for leading X-ray observatories to closely follow G2 on its way to
    the nucleus.
article_number: '221102'
article_processing_charge: No
article_type: original
arxiv: 1
author:
- first_name: Imre
  full_name: Bartos, Imre
  last_name: Bartos
- first_name: Zoltán
  full_name: Haiman, Zoltán
  id: 7c006e8c-cc0d-11ee-8322-cb904ef76f36
  last_name: Haiman
- first_name: Bence
  full_name: Kocsis, Bence
  last_name: Kocsis
- first_name: Szabolcs
  full_name: Márka, Szabolcs
  last_name: Márka
citation:
  ama: Bartos I, Haiman Z, Kocsis B, Márka S. Gas cloud G2 can illuminate the black
    hole population near the galactic center. <i>Physical Review Letters</i>. 2013;110(22).
    doi:<a href="https://doi.org/10.1103/physrevlett.110.221102">10.1103/physrevlett.110.221102</a>
  apa: Bartos, I., Haiman, Z., Kocsis, B., &#38; Márka, S. (2013). Gas cloud G2 can
    illuminate the black hole population near the galactic center. <i>Physical Review
    Letters</i>. American Physical Society. <a href="https://doi.org/10.1103/physrevlett.110.221102">https://doi.org/10.1103/physrevlett.110.221102</a>
  chicago: Bartos, Imre, Zoltán Haiman, Bence Kocsis, and Szabolcs Márka. “Gas Cloud
    G2 Can Illuminate the Black Hole Population near the Galactic Center.” <i>Physical
    Review Letters</i>. American Physical Society, 2013. <a href="https://doi.org/10.1103/physrevlett.110.221102">https://doi.org/10.1103/physrevlett.110.221102</a>.
  ieee: I. Bartos, Z. Haiman, B. Kocsis, and S. Márka, “Gas cloud G2 can illuminate
    the black hole population near the galactic center,” <i>Physical Review Letters</i>,
    vol. 110, no. 22. American Physical Society, 2013.
  ista: Bartos I, Haiman Z, Kocsis B, Márka S. 2013. Gas cloud G2 can illuminate the
    black hole population near the galactic center. Physical Review Letters. 110(22),
    221102.
  mla: Bartos, Imre, et al. “Gas Cloud G2 Can Illuminate the Black Hole Population
    near the Galactic Center.” <i>Physical Review Letters</i>, vol. 110, no. 22, 221102,
    American Physical Society, 2013, doi:<a href="https://doi.org/10.1103/physrevlett.110.221102">10.1103/physrevlett.110.221102</a>.
  short: I. Bartos, Z. Haiman, B. Kocsis, S. Márka, Physical Review Letters 110 (2013).
date_created: 2024-09-06T07:48:38Z
date_published: 2013-05-30T00:00:00Z
date_updated: 2024-09-25T08:25:00Z
day: '30'
doi: 10.1103/physrevlett.110.221102
extern: '1'
external_id:
  arxiv:
  - '1302.3220'
intvolume: '       110'
issue: '22'
language:
- iso: eng
main_file_link:
- open_access: '1'
  url: ' https://doi.org/10.48550/arXiv.1302.3220'
month: '05'
oa: 1
oa_version: Preprint
publication: Physical Review Letters
publication_identifier:
  issn:
  - 0031-9007
  - 1079-7114
publication_status: published
publisher: American Physical Society
quality_controlled: '1'
scopus_import: '1'
status: public
title: Gas cloud G2 can illuminate the black hole population near the galactic center
type: journal_article
user_id: 317138e5-6ab7-11ef-aa6d-ffef3953e345
volume: 110
year: '2013'
...
