activity
19962019
most citedA terrestrial planet candidate in a temperate orbit around Proxima Centauri

1.3k citations · 1.6k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.EP2019★ 25 cited

Frequency of planets orbiting M dwarfs in the Solar neighbourhood

M. Tuomi, H. R. A. Jones, R. P. Butler +14

The most abundant stars in the Galaxy, M dwarfs, are very commonly hosts to diverse systems of low-mass planets. Their abundancy implies that the general occurrence rate of planets…

astro-ph.SR2018★ 27 cited

Stellar activity analysis of Barnard's Star: Very slow rotation and evidence for long-term activity cycle

B. Toledo-Padrón, J. I. González Hernández, C. Rodríguez-López +58

The search for Earth-like planets around late-type stars using ultra-stable spectrographs requires a very precise characterization of the stellar activity and the magnetic cycle of…

astro-ph.EP2018★ 142 cited

A candidate super-Earth planet orbiting near the snow line of Barnard's star

I. Ribas, M. Tuomi, A. Reiners +60

At a distance of 1.8 parsecs, Barnard's star (Gl 699) is a red dwarf with the largest apparent motion of any known stellar object. It is the closest single star to the Sun, second…

astro-ph.EP2018★ 32 cited

AD Leonis: Radial velocity signal of stellar rotation or spin-orbit resonance?

Mikko Tuomi, Hugh R. A. Jones, Guillem Anglada-Escudé +3

AD Leonis is a nearby magnetically active M dwarf. We find Doppler variability with a period of 2.23 days as well as photometric signals: (1) a short period signal which is similar…

astro-ph.EP2016★ 1.3k cited

A terrestrial planet candidate in a temperate orbit around Proxima Centauri

Guillem Anglada-Escudé, Pedro J. Amado, John Barnes +28

At a distance of 1.295 parsecs, the red-dwarf Proxima Centauri ( Centauri C, GL 551, HIP 70890, or simply Proxima) is the Sun's closest stellar neighbor and one of the best stud…

astro-ph.SR2015★ 38 cited

Fast radio bursts: the observational case for a Galactic origin

Dan Maoz, Abraham Loeb, Yossi Shvartzvald +10

There are by now ten published detections of fast radio bursts (FRBs), single bright GHz-band millisecond pulses of unknown origin. Proposed explanations cover a broad range from e…

astro-ph.SR2015★ 17 cited

Model computations of blue stragglers and W UMa-type stars in globular clusters

Kazimierz Stepien, Marcin Kiraga

It was recently demonstrated that contact binaries occur in globular clusters (GCs) only immediately below turn-off point and in the region of blue straggler stars (BSs). In additi…

astro-ph.SR2014

Evolution of Cool Close Binaries -- Rapid Mass Transfer and Near Contact Binaries

Kazimierz Stepien, Marcin Kiraga

[Abridged] We test the evolutionary model of cool close binaries on the observed properties of near contact binaries (NCBs). Those with a more massive component filling the Roche l…

astro-ph.SR2013★ 4 cited

ASAS Photometry of ROSAT Sources. II.New Variables from the ASAS North Survey

M. Kiraga, K. Stepien

We present a catalog of 307 optical counterparts of the bright ROSAT X-ray sources, identified with the ASAS North survey data and showing periodic brightness variations. They all…

astro-ph.SR2012

ASAS photometry of ROSAT sources I. Periodic variable stars coincident with bright sources from ROSAT all sky survey

M. Kiraga

Photometric data from the ASAS - South (declination less than 29 deg) survey have been used for identification of bright stars located near the sources from the ROSAT All Sky Surve…

astro-ph2007★ 16 cited

Age-Rotation-Activity Relations for M Dwarf Stars Based on ASAS Photometric Data

M. Kiraga, K. Stepien

Based on analysis of photometric observations of nearby M type stars obtained with ASAS, 31 periodic variables were detected. The determined periods are assumed to be related to ro…

astro-ph2000★ 17 cited

Gaussianity of Cosmic Velocity Fields and Linearity of the Velocity-Gravity Relation

Pawel Ciecielag, Michal Chodorowski, Marcin Kiraga +3

We present a numerical study of the relation between the cosmic peculiar velocity field and the gravitational acceleration field. We show that on mildly non-linear scales (4-10 Mpc…

astro-ph1996★ 21 cited

The Color--Magnitude Diagram in Baade's Window Revisited

M. Kiraga, B. Paczynski, K. Z. Stanek

We have reanalyzed the OGLE and photometry of stars in Baade's Window, and we confirm the extinction map published by Stanek (1996). However, we find that th…