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researcher

T. Ak

19 papers hereh-index 14491 citations69 works total

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

author position
  • first author4
  • middle author9
  • last author4

Across the 17 of 19 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA9
  • astro-ph4
  • astro-ph.SR4
  • astro-ph.EP1
  • astro-ph.HE1
same name
  • T. Ak — 28 papers, h 11
  • T. Ak — 1 paper
  • T. Ak — 1 paper, h 0

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
20052023
most citedSpatial distribution and galactic model parameters of cataclysmic variables

49 citations · 411 across the 19 of their papers we have counts for

collaborators
Showing astro-phShow all

4 papers · 1 filter

astro-ph2007★ 49 cited

Spatial distribution and galactic model parameters of cataclysmic variables

T. Ak, S. Bilir, S. Ak +1

The spatial distribution, galactic model parameters and luminosity function of cataclysmic variables (CVs) in the solar neighbourhood have been determined from a carefully establis…

astro-ph2007★ 28 cited

A new absolute magnitude calibration with 2MASS for cataclysmic variables

T. Ak, S. Bilir, S. Ak +1

Using reliable trigonometric measurements, we find that the absolute magnitude of cataclysmic variables depends on the orbital period and de-reddened (J−H)0​ and $(H-K_{s})_{0}…

astro-ph2005★ 18 cited

The orbital period of Nova V2540 Ophiuchi (2002)

T. Ak, A. Retter, A. Liu

We present the results of 26 nights of CCD photometry of the nova V2540 Oph (2002) from 2003 and 2004. We find a period of 0.284781 +/- 0.000006 d (6.8347 +/- 0.0001 h) in the data…

astro-ph2005★ 8 cited

A photometric study of V1193 Ori: detection of orbital and negative superhump periods

T. Ak, A. Retter, A. Liu

We present the results obtained from unfiltered photometric CCD observations of V1193 Ori made during 24 nights between November 2002 and January 2003. We found periods of 0.1430 d…

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