Search Results - "Getman, Konstantin V."
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X-Ray Superflares from Pre-main-sequence Stars: Flare Energetics and Frequency
Published in The Astrophysical journal (01-07-2021)“…Abstract Solar-type stars exhibit their highest levels of magnetic activity during their early convective pre-main-sequence (PMS) phase of evolution. The most…”
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Magnetic Activity–Rotation–Age–Mass Relations in Late-pre-main-sequence Stars
Published in The Astrophysical journal (01-07-2023)“…Abstract We study the four-dimensional relationships between magnetic activity, rotation, mass, and age for solar-type stars in the age range 5–25 Myr. This is…”
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CORE-HALO AGE GRADIENTS AND STAR FORMATION IN THE ORION NEBULA AND NGC 2024 YOUNG STELLAR CLUSTERS
Published in The Astrophysical journal (01-06-2014)“…We analyze age distributions of two nearby rich stellar clusters, the NGC 2024 (Flame Nebula) and Orion Nebula cluster (ONC) in the Orion molecular cloud…”
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X-Ray Superflares from Pre-main-sequence Stars: Flare Modeling
Published in The Astrophysical journal (01-10-2021)“…Abstract Getman et al. report the discovery, energetics, frequencies, and effects on environs of >1000 X-ray superflares with X-ray energies E X ∼ 10 34 –10 38…”
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THE SPATIAL STRUCTURE OF YOUNG STELLAR CLUSTERS. I. SUBCLUSTERS
Published in The Astrophysical journal (01-06-2014)“…The clusters of young stars in massive star-forming regions show a wide range of sizes, morphologies, and numbers of stars. Their highly subclustered…”
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X-Ray, Near-ultraviolet, and Optical Flares Produced by Colliding Magnetospheres in the Young High-eccentricity Binary DQ Tau
Published in The Astrophysical journal (01-12-2023)“…Abstract DQ Tau is a unique young high-eccentricity binary system that exhibits regular magnetic reconnection flares and pulsed accretion near periastron. We…”
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AGE GRADIENTS IN THE STELLAR POPULATIONS OF MASSIVE STAR FORMING REGIONS BASED ON A NEW STELLAR CHRONOMETER
Published in The Astrophysical journal (01-06-2014)“…A major impediment to understanding star formation in massive star-forming regions (MSFRs) is the absence of a reliable stellar chronometer to unravel their…”
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THE SPATIAL STRUCTURE OF YOUNG STELLAR CLUSTERS. III. PHYSICAL PROPERTIES AND EVOLUTIONARY STATES
Published in The Astrophysical journal (20-10-2015)“…ABSTRACT We analyze the physical properties of stellar clusters that are detected in massive star-forming regions in the MYStIX project-a comparative,…”
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XUE: Molecular Inventory in the Inner Region of an Extremely Irradiated Protoplanetary Disk
Published in Astrophysical journal. Letters (01-12-2023)“…Abstract We present the first results of the eXtreme UV Environments (XUE) James Webb Space Telescope (JWST) program, which focuses on the characterization of…”
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X-Ray Flares in Orion Young Stars. II. Flares, Magnetospheres, and Protoplanetary Disks
Published in The Astrophysical journal (20-11-2008)“…We study the properties of powerful X-ray flares from 161 pre-main- sequence (PMS) stars observed with the Chandra X-ray Observatory in the Orion Nebula…”
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Kinematics in Young Star Clusters and Associations with Gaia DR2
Published in The Astrophysical journal (01-01-2019)“…The Gaia mission has opened a new window into the internal kinematics of young star clusters at the sub-km s−1 level, with implications for our understanding…”
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THE SPATIAL STRUCTURE OF YOUNG STELLAR CLUSTERS. II. TOTAL YOUNG STELLAR POPULATIONS
Published in The Astrophysical journal (23-03-2015)“…ABSTRACT We investigate the intrinsic stellar populations (estimated total numbers of OB and pre-main-sequence stars down to 0.1 ) that are present in 17…”
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Evolution of X-Ray Activity in <25 Myr Old Pre-main Sequence Stars
Published in The Astrophysical journal (01-08-2022)“…Measuring the evolution of X-ray emission from pre-main-sequence (PMS) stars gives insight into two issues: the response of magnetic dynamo processes to…”
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Innovations in the Analysis of Chandra-ACIS Observations
Published in The Astrophysical journal (10-05-2010)“…As members of the instrument team for the Advanced CCD Imaging Spectrometer (ACIS) on NASA's Chandra X-ray Observatory and as Chandra General Observers, we…”
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The Effect of Molecular Cloud Properties on the Kinematics of Stars Formed in the Trifid Region
Published in The Astrophysical journal (01-09-2022)“…Abstract The dynamical states of molecular clouds may affect the properties of the stars they form. In the vicinity of the Trifid Nebula ( d = 1180 ± 25 pc),…”
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X-Ray Flares in Orion Young Stars. I. Flare Characteristics
Published in The Astrophysical journal (20-11-2008)“…Pre-main-sequence (PMS) stars are known to produce powerful X-ray flares, which resemble magnetic reconnection solar flares scaled by factors up to 10…”
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The Elephant Trunk Nebula and the Trumpler 37 cluster: contribution of triggered star formation to the total population of an HII region
Published in Monthly notices of the Royal Astronomical Society (11-11-2012)“…Abstract Rich young stellar clusters produce H ii regions whose expansion into the nearby molecular cloud is thought to trigger the formation of new stars…”
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YOUNG STELLAR POPULATIONS IN MYStIX STAR-FORMING REGIONS: CANDIDATE PROTOSTARS
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT The Massive Young Star-Forming Complex in Infrared and X-ray (MYStIX) project provides a new census on stellar members of massive star-forming regions…”
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A Chandra Observation of the Obscured Star-forming Complex W40
Published in The Astrophysical journal (20-12-2010)“…The young stellar cluster illuminating the W40 H II region, one of the nearest massive star-forming regions, has been observed with the ACIS detector on board…”
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The Elephant Trunk Nebula and the Trumpler 37 cluster: contribution of triggered star formation to the total population of an H ii region
Published in Monthly notices of the Royal Astronomical Society (11-11-2012)“…ABSTRACT Rich young stellar clusters produce H ii regions whose expansion into the nearby molecular cloud is thought to trigger the formation of new stars…”
Get full text
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