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相关论文: Explaining the Praesepe blue straggler HD 73666

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Blue metal-poor (BMP) stars are the main-sequence stars that appear bluer and more luminous than normal turn-off stars of metal-poor globular clusters. They are believed to be either field blue straggler stars (FBSS) formed via post-mass…

太阳与恒星天体物理 · 物理学 2023-08-16 Anju Panthi , Annapurni Subramaniam , Kaushar Vaidya , Vikrant Jadhav , Sharmila Rani , Sivarani Thirupathi , Sindhu Pandey

We show that the X-ray source W31 in the core of the globular cluster 47 Tucanae is physically associated with the bright blue straggler BSS-7. The two sources are astrometrically matched to 0.061\arcsec, with a chance coincidence…

天体物理学 · 物理学 2009-11-13 C. Knigge , R. L. Gilliland , A. Dieball , D. R. Zurek , M. M. Shara , K. S. Long

Stripped stars are a common product of binary stellar systems and span a wide mass range from Wolf-Rayet stars to hot subdwarfs and helium white dwarfs. The recent discovery of intermediate-mass stripped stars, with masses between those of…

太阳与恒星天体物理 · 物理学 2026-05-25 Annachiara Picco , Pablo Marchant , Daniel Pauli , Hugues Sana

Blue Straggler stars are present in all the properly observed Globular Clusters. They mimic a rejuvenated stellar population and their existence has been a puzzle for many years. We performed an extensive spectroscopic survey of the surface…

太阳与恒星天体物理 · 物理学 2013-01-16 Loredana Lovisi , Alessio Mucciarelli , Barbara Lanzoni , Francesco R. Ferraro , Emanuele Dalessandro

We investigate the old open cluster M67 using ultraviolet photometric data of Ultra-Violet Imaging Telescope in multi-filter far-UV bands. M67, well known for the presence of several blue straggler stars (BSS), has been put to detailed…

Stellar mergers are estimated to be common events in the Galaxy. The best studied stellar merger case to date is V1309 Sco (= Nova Scorpii 2008) which was originally misclassified as a Nova event. Later identified as the merger of the…

(Abridged). One of the most metal-deficient blue compact galaxies (BCGs) HS 0822+3542 (Z=1/34 Zsun), is also one of the nearest such objects. A trigger mechanism for its current SF burst has remained unclear. We report the discovery of a…

天体物理学 · 物理学 2009-11-10 S. A. Pustilnik , A. Y. Kniazev , A. G. Pramskij , A. V. Ugryumov , J. Masegosa

Recently, several non-interacting black hole-stellar binaries have been identified in Gaia data. For example, Gaia BH1, where a Sun-like star is in a moderate eccentricity (e=0.44), 185-day orbit around a black hole. This orbit is difficult…

太阳与恒星天体物理 · 物理学 2025-04-23 A. Generozov , H. B. Perets

The stellar populations in a stellar complex in NGC 6946 are analyzed on images taken with the Wide Field Planetary Camera 2 on board the Hubble Space Telescope. The complex is peculiar by its very high density of stars and clusters and…

天体物理学 · 物理学 2009-11-07 S. S. Larsen , Yu. N. Efremov , B. G. Elmegreen , E. J. Alfaro , P. Battinelli , P. W. Hodge , T. Richtler

We present a quantitative study on the properties at death of fast-rotating massive stars evolved at low-metallicity, objects that are proposed as likely progenitors of long-duration gamma-ray bursts (LGRBs). We perform 1D+rotation…

高能天体物理现象 · 物理学 2013-01-31 Luc Dessart , Evan O'Connor , Christian D. Ott

Blue straggler stars (BSSs) are believed to form through mass transfer in binary systems or stellar collisions. The reported presence of double BSS sequences in some globular clusters (GCs) has been interpreted as evidence that these two…

The formation of hot subdwarf stars is still unclear. Both single-star and binary scenarios have been proposed to explain the properties of these evolved stars situated at the extreme blue end of the horizontal branch. The observational…

太阳与恒星天体物理 · 物理学 2015-06-12 S. Geier

We explore mechanisms for the regulation of star formation in dwarf galaxies. We concentrate primarily on a sample in the Virgo cluster, which has HI and blue total photometry, for which we collected H$\alpha$ data at the Wise Observatory.…

天体物理学 · 物理学 2009-10-30 Noah Brosch , Ana Heller , Elchanan Almoznino

We report the results of photometric monitoring of the Melotte 66 field in BVI filters. Ten variables were identified with nine being new discoveries. The sample includes eight eclipsing binaries of which four are W UMa type stars, one star…

天体物理学 · 物理学 2009-11-13 K. Zloczewski , J. Kaluzny , W. Krzeminski , A. Olech , I. B. Thompson

We present multi-epoch infrared photometry and spectroscopy obtained with warm Spitzer, Subaru and SOFIA to assess variability for the young ($\sim$20 Myr) and dusty debris systems around HD 172555 and HD 113766A. No variations (within…

地球与行星天体物理 · 物理学 2020-07-29 Kate Y. L. Su , George H. Rieke , Carl Melis , Alan P. Jackson , Paul S. Smith , Huan Y. A. Meng , Andras Gaspar

We recently discovered a large number of highly active Be stars in the open cluster NGC 3766, making it an excellent location to study the formation mechanism of Be star disks. To explore whether similar disk appearances and/or…

太阳与恒星天体物理 · 物理学 2009-07-22 M. Virginia McSwain , Wenjin Huang , Douglas R. Gies

Binary systems can evolve into immensely different exotic systems such as blue straggle stars (BSSs), yellow straggler stars, cataclysmic variables, type Ia supernovae depending on their initial mass, the orbital parameters and evolution.…

太阳与恒星天体物理 · 物理学 2022-07-11 Vikrant V. Jadhav

Binaries consisting of a pulsar and a black hole (BH) are a holy grail of astrophysics, both for their significance for stellar evolution and for their potential application as probes of strong gravity. In spite of extensive surveys of our…

高能天体物理现象 · 物理学 2015-05-20 C. -A. Faucher-Giguere , Abraham Loeb

Blue straggler star (BSS) candidates have been observed in all old dwarf spheroidal galaxies (dSphs), however whether or not they are authentic BSSs or young stars has been a point of debate. To both address this issue and obtain a better…

天体物理学 · 物理学 2009-11-13 M. Mapelli , E. Ripamonti , E. Tolstoy , S. Sigurdsson , M. J. Irwin , G. Battaglia

Substellar objects, like planets and brown dwarfs orbiting stars, are by-products of the star formation process. The evolution of their host stars may have an enourmous impact on these small companions. Vice versa a planet might also…

太阳与恒星天体物理 · 物理学 2015-05-13 S. Geier , H. Edelmann , U. Heber , L. Morales-Rueda