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It remains unclear whether massive star evolution is facilitated by mass loss through stellar winds only, or whether episodic mass loss during an eruptive luminous blue variable (LBV) phase is also significant. LBVs exhibit unique…

太阳与恒星天体物理 · 物理学 2018-10-10 V. M. Kalari , J. S. Vink , P. L. Dufton , M. Fraser

Hypervelocity stars (HVS) traverse the Galaxy from the central black hole to the outer halo. We show that the Galactic potential within 200 pc acts as a high pass filter preventing low velocity HVS from reaching the halo. To trace the…

天体物理学 · 物理学 2009-11-13 S. J. Kenyon , B. C. Bromley , M. J. Geller , W. R. Brown

Luminous Blue Variables (LBVs) are enigmatic, evolved, massive stars. Their variability has been observed to be episodic with large eruptions, along with variations on time-scales of days to decades. We have extracted light curves of 37…

太阳与恒星天体物理 · 物理学 2025-01-03 Becca Spejcher , Noel D. Richardson , Herbert Pablo , Marina Beltran , Payton Butler , Eddie Avila

We present the results of a study of the star HD 34736. The spectropolarimetric observations carried out at the 6-m telescope showed the presence of a strong variable longitudinal magnetic field, exceeding -4500 G. The analysis of the…

太阳与恒星天体物理 · 物理学 2015-06-19 E. A. Semenko , I. I. Romanyuk , D. O. Kudryavtsev , I. A. Yakunin

The O- and B-type (OB-type) pulsating stars are important objects to study the structure and evolution of massive stars through asteroseismology. A large amount of data from various sky surveys provide an unprecedented opportunity to search…

太阳与恒星天体物理 · 物理学 2024-12-06 Xiang-dong Shi , Sheng-bang Qian , Li-ying Zhu , Liang Liu , Lin-jia Li , Lei Zang

This paper reports the results from the multicolor photometric observations of 15 pre-main sequence stars collected in the period 2010 September - 2017 October. The stars from our study are located in the star-forming HII region IC 5070.…

太阳与恒星天体物理 · 物理学 2018-11-07 Sunay Ibryamov , Evgeni Semkov , Teodor Milanov , Stoyanka Peneva

The spectroscopic and photometric analysis of sample Am stars are carried out to determine the stellar characteristics of each studied star. The CCD photometric analysis of HD 98851 and HD 207561 show clear evidence of pulsation variability…

太阳与恒星天体物理 · 物理学 2019-09-17 Gireesh C. Joshi

This work presents the first large-scale photometric variability survey of the intermediate age (~200 Myr) open cluster M11. Thirteen nights of data over two observing seasons were analyzed (using crowded field and ensemble photometry…

天体物理学 · 物理学 2008-11-26 Jonathan R. Hargis , Eric L. Sandquist , David H. Bradstreet

We analyze Keck ESI spectroscopy of HVS17, a B-type star traveling with a Galactic rest frame radial velocity of +445 km/s in the outer halo of the Milky Way. HVS17 has the projected rotation of a main sequence B star and is chemically…

太阳与恒星天体物理 · 物理学 2015-06-16 Warren R. Brown , Judith G. Cohen , Margaret J. Geller , Scott J. Kenyon

A radial velocity (RV) survey to detect central stars in binary systems was carried out between 2002 and 2004. De Marco et al. (2004) reported that 10 out of 11 monitored stars exhibited strong RV variability, but periods were not detected.…

天体物理学 · 物理学 2007-09-12 Orsola De Marco , S. Wortel , Howard E. Bond , Dianne Harmer

Heartbeat stars (HB stars) are a class of eccentric binary stars with close periastron passages. The characteristic photometric HB signal evident in their light curves is produced by a combination of tidal distortion, heating, and Doppler…

Context: [abbreviated] Aims: Kepler data of three known Be stars are re-visited to establish their pulsational nature and assess the properties of additional, non-pulsational variations. The three program stars turned out to be one inactive…

太阳与恒星天体物理 · 物理学 2016-10-05 Thomas Rivinius , Dietrich Baade , Alex Carciofi

We report the discovery of 5 new Herbig Ae/Be candidate stars in the Small Magellanic Cloud in addition to the 2 reported in Beaulieu et al. (2001). We discuss these 7 HAeBe candidate stars in terms of (1) their irregular photometric…

天体物理学 · 物理学 2009-11-10 W. J. de Wit , J-P. Beaulieu , H. J. G. L. M. Lamers , E. Lesquoy , J-B. Marquette , ;

Stellar oscillations are an important tool to probe the interior of a star. Subdwarf B stars are core helium burning objects, but their formation is poorly understood as neither single star nor binary evolution can fully explain their…

天体物理学 · 物理学 2009-11-13 A. Tillich , U. Heber , S. J. O'Toole , R. Østensen , S. Schuh

We use data from the Transiting Exoplanet Survey Satellite (TESS) to search for, and set limits on, optical to near-infrared photometric variability of the well-vetted, candidate James Webb Space Telescope (JWST) spectrophotometric…

We carried out spectroscopic observations with Subaru/HDS of 50 solar-type superflare stars found from Kepler data. More than half (34 stars) of the target stars show no evidence of the binary system, and we confirmed atmospheric parameters…

太阳与恒星天体物理 · 物理学 2017-02-16 Yuta Notsu , Satoshi Honda , Hiroyuki Maehara , Shota Notsu , Takuya Shibayama , Daisaku Nogami , Kazunari Shibata

This study presents an investigation of nearly two dozen candidate Luminous Blue Variables (cLBVs) in the galaxies M31 and M33. Eight stars have been studied in detail, while an additional sixteen objects are briefly mentioned. Multi-epoch…

太阳与恒星天体物理 · 物理学 2026-03-12 Sai Li , Cheng Liu , Jincheng Guo

This paper describes the first part of the photometric data from the 9x9 deg ASAS cameras monitoring the whole southern hemisphere in V-band. Data acquisition and reduction pipeline is described and preliminary list of variable stars is…

天体物理学 · 物理学 2009-07-09 G. Pojmanski

Halo stars with unusually high radial velocity ("hypervelocity" stars, or HVS) are thought to be stars unbound to the Milky Way that originate from the gravitational interaction of stellar systems with the supermassive black hole at the…

天体物理学 · 物理学 2009-11-13 Mario G. Abadi , Julio F. Navarro , Matthias Steinmetz

We present a study of the variation timescales of the chromospheric activity indicator H$\alpha$ on a sample of 13 fully-convective, active mid-to-late M stars with masses between 0.1--0.3 solar masses. Our goal was to determine the…

太阳与恒星天体物理 · 物理学 2022-04-13 Amber A. Medina , David Charbonneau , Jennifer G. Winters , Jonathan Irwin , Jessica Mink