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We report on a high-resolution, spectroscopic stellar parameter and abundance analysis of a d' symbiotic star: the yellow component of StH\alpha190. This star has recently been discovered, and confirmed here, to be a rapidly rotating…

天体物理学 · 物理学 2009-11-06 Verne V. Smith , Claudio B. Pereira , Katia Cunha

High resolution data in the region of the line Halpha have been obtained at the time of the light maximum and after it of the 2006 optical outburst of the symbiotic binary Z And. A blue-shifted absorption component indicating outflow…

天体物理学 · 物理学 2008-11-26 N. A. Tomov , M. T. Tomova , D. V. Bisikalo

We report finding high-velocity components in the H{\alpha} emission wings of St 2-22 spectra, obtained in 2005. This discovery have encouraged us to start the present study, aiming to show that this little studied object is a jet producing…

太阳与恒星天体物理 · 物理学 2018-10-24 T. Tomov , R. Zamanov , C. Gałan , P. Pietrukowicz

The spectral signature of collimated bipolar jets have been discovered on high resolution spectra of Hen 3-1341 during the 1999 outburst, the first ever recorded for this symbiotic star. The jets show up as emission components at DeltaRV =…

天体物理学 · 物理学 2007-05-23 Toma Tomov , Ulisse Munari , Paola Marrese

We present high-dispersion echelle spectroscopic observations and a narrow-band [N II] image of the remarkable jet-like features of He 2-90. They are detected in the echelle spectra in the H-alpha and [N II] lines but not in other nebular…

天体物理学 · 物理学 2009-11-07 Martin A. Guerrero , Luis F. Miranda , You-Hua Chu , Monica Rodriguez , Rosa M. Williams

We have observed the bipolar jet from RW Aur A with STIS on board the HST. After continuum subtraction, morphological and kinematic properties of this outflow can be traced to within 0."1 from the source in forbidden emission lines. The jet…

天体物理学 · 物理学 2009-11-07 Jens Woitas , Thomas P. Ray , Francesca Bacciotti , Christopher J. Davis , Jochen Eisl"offel

Using the partially completed Submillimeter Array with five antennas, we have observed the CO J=2-1 and 3-2 emission from the envelope surrounding the carbon star V Hya. The high-angular resolution (2"-4") maps show that V Hya is powering a…

From 1994 to 1997 we monitored the optical spectrum of RXJ0019.8+2156. This supersoft X-ray source is one of only two accreting white dwarfs in the Galaxy thought to be burning hydrogen on their surface as a consequence of a high rate of…

天体物理学 · 物理学 2009-10-30 C. M. Becker , R. A. Remillard , S. A. Rappaport , J. E. McClintock

We present an analysis of high resolution spectral observations of the symbiotic star StHa 190. A 30 days period has been derived from radial velocities of the G-type absorption lines and the HeII 4686A emission line. The main aim of this…

太阳与恒星天体物理 · 物理学 2011-02-28 M. Cikała , M. Mikołajewski , T. Tomov , D. Kolev , L. Georgiev , U. Munari , P. Marrese , T. Zwitter

The atmosphere of the extremely high-velocity (530-920 km/s) early B-type star HD271791 is enriched in $\alpha$-process elements, which suggests that this star is a former secondary component of a massive tight binary system and that its…

太阳与恒星天体物理 · 物理学 2009-04-13 V. V. Gvaramadze

We have studied optical spectra of the symbiotic star Z And, obtained during its latest outburst started in April 2006, with the aim of finding changes in the spectrum yielding clues to the nature of the hot component and its outbursts. The…

天体物理学 · 物理学 2009-11-11 Mari Burmeister , Laurits Leedjarv

Optical images and high-dispersion spectra have been obtained of the ejected material surrounding the pulsating AGB star Mira A. The two streams of knots on either side of the star, found in far ultra-viollet (FUV) GALEX images, have now…

星系天体物理 · 物理学 2015-05-13 J. Meaburn , J. A. Lopez , P. Boumis , M. Lloyd , M. P. Redman

New spectroscopic observations of the halo hyper-velocity star candidate SDSS J121150.27+143716.2 ($V=17.92$ mag) revealed a cool companion to the hot subdwarf primary. The components have a very similar radial velocity and their absolute…

太阳与恒星天体物理 · 物理学 2016-04-13 Péter Németh , Eva Ziegerer , Andreas Irrgang , Stephan Geier , Felix Fürst , Thomas Kupfer , Ulrich Heber

The object of this study is one of the most energetic and luminous molecular outflows known in the Galaxy, G331.512-0.103. Observations with ALMA Band 7 (350 GHz; 0.86 mm) reveal a very compact, extremely young bipolar outflow and a more…

We present narrow-band optical images, VLA-A 3.6 cm continuum and H92alpha emission line data and high resolution long-slit [N II] spectra of Hu 2-1. The formation of Hu 2-1 appears dominated by anisotropic mass ejection during the late AGB…

天体物理学 · 物理学 2009-10-31 Luis F. Miranda , Jose M. Torrelles , Martin A. Guerrero , Roberto Vazquez , Yolanda Gomez

We present evidence that the spectroscopically identified bipolar jets of the pre-main sequence binary KH 15D are a common product of the whole binary system, rather than being launched from either star individually. They may be launched…

太阳与恒星天体物理 · 物理学 2015-05-14 Reinhard Mundt , Catrina M. Hamilton , William Herbst , Christopher M. Johns-Krull , Joshua N. Winn

Yellow symbiotic stars are useful targets to probe whether mass transfer has happened in these binary systems. However, the number of known yellow symbiotic stars is very scarce. We report spectroscopic observations of five candidate yellow…

太阳与恒星天体物理 · 物理学 2016-04-13 N. O. Baella , C. B. Pereira , L. F. Miranda , A. Alvarez-Candal

St 2-22 is a relatively poorly studied S-type symbiotic system that belongs to a small group of jet-producing systems as a result of disc accretion onto a white dwarf fed by its red giant companion. The goal of this paper is to analyse the…

太阳与恒星天体物理 · 物理学 2022-01-26 Cezary Galan , Joanna Mikolajewska , Krystian Ilkiewicz , Berto Monard , Szymon T. Zywica , Radoslav K. Zamanov

The 24 M Jupiter mass brown dwarf 2MASS1207-3932 has for some time been known to show clear signs of classical T Tauri-like accretion. Through analysis of its oxygen forbidden emission we have discovered that it is driving a bipolar…

天体物理学 · 物理学 2009-11-13 E. T. Whelan , T. P. Ray , S. Randich , F. Baciotti , R. Jayawardhana , L. Testi , A. Natta , S. Mohanty

A mysterious X-ray-emitting object has been detected moving away from the high-mass gamma-ray binary PSR B1259-63, which contains a non-accreting pulsar and a Be star whose winds collide forming a complex interaction structure. Given the…

高能天体物理现象 · 物理学 2015-12-16 Maxim V. Barkov , Valenti Bosch-Ramon
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