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M. Torres

34 papers hereh-index 15756 citations50 works total

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

author position
  • first author1
  • middle author20
  • last author1

Across the 22 of 34 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE24
  • astro-ph.SR6
  • astro-ph.GA4
same name
  • M. Torres — 282 papers, h 65
  • M. Torres — 52 papers, h 26
  • M. Torres — 52 papers, h 18
  • M. Torres — 40 papers, h 4
  • M. Torres — 32 papers, h 12
  • M. Torres — 21 papers, h 8

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
20092026
most citedThe mass function of GX 339-4 from spectroscopic observations of its donor star

108 citations · 776 across the 34 of their papers we have counts for

collaborators
Showing 2012 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2012★ 18 cited

CXOGBSJ174444.7-260330: a new long orbital period cataclysmic variable in a low state

E. M. Ratti, T. F. J. van Grunsven, P. G. Jonker +12

We present phase-resolved spectroscopy and photometry of a source discovered with the Chandra Galactic Bulge Survey (GBS), CXOGBSJ174444.7-260330 (aka CX93 and CX153 in the previou…

astro-ph.HE2012★ 37 cited

The nature of the bright ULX X-2 in NGC3921: a Chandra position and HST candidate counterpart

P. G. Jonker, M. Heida, M. A. P. Torres +6

We report on Chandra observations of the bright ultra-luminous X-ray (ULX) source in NGC3921. Previous XMM observations reported in the literature show the presence of a bright ULX…

astro-ph.HE2012★ 84 cited

The black hole candidate XTE J1752-223 towards and in quiescence: optical and simultaneous X-ray - radio observations

E. M. Ratti, P. G. Jonker, J. C. A. Miller-Jones +10

We present optical, X-ray and radio observations of the black hole transient (BHT) XTE J1752-223 towards and in quiescence. Optical photometry shows that the quiescent magnitude of…

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