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相关论文: New luminous blue variable candidates in the NGC 2…

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SN2002kg is a type IIn supernova, detected in October 2002 in the nearby spiral galaxy NGC 2403. We show that the position of SN2002kg agrees within the errors with the position of the LBV V37. Ground based and HST ACS images however show…

天体物理学 · 物理学 2009-11-10 Kerstin Weis , Dominik J. Bomans

The planetary nebula (PN) IC 4997 is one of a few rapidly evolving objects with variable brightness and nebular emission around a hydrogen-deficient star. In this study, we have determined the physical conditions and chemical abundances of…

太阳与恒星天体物理 · 物理学 2022-06-17 A. Danehkar , M. Parthasarathy

BL Lac objects are known to have compact jets inclined to our line of sight at a small angle, showing prominent radio emission. Two radio-weak BL Lac candidates with no counterparts in current radio surveys were recently reported by Massaro…

星系天体物理 · 物理学 2018-10-17 Hong-Min Cao , Sándor Frey , Krisztina É. Gabányi , Jun Yang , Lang Cui , Xiao-Yu Hong , Tao An

High resolution optical spectra (R = 60 000) of the LBV star P Cyg beyond outburst were obtained on the 6-meter BTA telescope in the wavelength range 477-780 nm. We perform a detailed identification of different types lines (photospheric…

太阳与恒星天体物理 · 物理学 2024-02-15 Valentina G. Klochkova , Vladimir E. Panchuk , Nonna S. Tavolzhanskaya

We present the results of high-resolution spectroscopy of the extremely luminous star CygOB2-No.12. We identified about 200 spectral features in the range 4552-7939 AA, including the interstellar NaI, KI lines and numerous very strong DIBs,…

太阳与恒星天体物理 · 物理学 2015-05-20 Valentina Klochkova , Eugene Chentsov , Anatoly Miroshnichenko

We present the results of a new epoch of a long-term photometric monitoring of the variable planetary nebula IC~4997. The integral $UBV$ light curves display a continuing brightening of 0.$^{m}15$ in $V$, a slight rise (<0.$^{m}1$) in $B$,…

太阳与恒星天体物理 · 物理学 2020-08-26 V. P. Arkhipova , M. A. Burlak , N. P. Ikonnikova , G. V. Komissarova , V. F. Esipov , V. I. Shenavrin

We measure the metallicity of the unusual hypervelocity star HE 0437-5439 from high resolution spectroscopy to be half-solar. We determine a spectral type of B2 IV-III for the star and derive an effective temperature Teff= 21,500 +/- 1,000…

天体物理学 · 物理学 2009-11-13 Alceste Z. Bonanos , Mercedes Lopez-Morales , Ian Hunter , Robert S. I. Ryans

The region surrounding the well-known reflection nebula, NGC 7023, illuminated by a Herbig Be star, HD 200775, located in the dark cloud L1174 is studied in this work. Based on the distances and proper motion values from Gaia DR2 of 20…

太阳与恒星天体物理 · 物理学 2020-05-04 Piyali Saha , Maheswar G. , Kamath U. S. , Lee C. W , Manoj P. , Blesson Mathew , Ekta Sharma

(Shortened) Luminous blue variable stars (LBVs) form dust as a result of episodic, violent mass loss. To investigate their contribution as dust producers in the Magellanic Clouds, we analyse 31 LBVs from a recent census. We built a…

太阳与恒星天体物理 · 物理学 2021-12-01 C. Agliozzo , N. Phillips , A. Mehner , D. Baade , P. Scicluna , F. Kemper , D. Asmus , W. -J. de Wit , G. Pignata

We present photoelectric and spectral observations of a hot candidate proto-planetary nebula - early B-type supergiant with emission lines in spectrum - IRAS 19336-0400. The light and color curves display fast irregular brightness…

太阳与恒星天体物理 · 物理学 2011-11-11 V. P. Arkhipova , M. A. Burlak , V. F. Esipov , N. P. Ikonnikova , G. V. Komissarova

The VISTA Variables in the Via Lactea (VVV) survey obtained near-infrared photometry toward the Galactic bulge and the southern disc plane for a decade (2010 - 2019). We designed a modified Lomb-Scargle method to search for large-amplitude…

Aiming to perform a study of the warm dust and gas in the luminous blue variable star G79.29+0.46 and its associated nebula, we present infrared Spitzer imaging and spectroscopy, and new CO J=2-->1 and 4-->3 maps obtained with the IRAM 30m…

太阳与恒星天体物理 · 物理学 2015-03-13 F. M. Jiménez-Esteban , J. R. Rizzo , Aina Palau

We present VI-band photometry for stars in the metal-rich globular cluster NGC 6496. Our time-series data were cadenced to search for long period variables (LPVs) over a span of nearly two years, and our variability search yielded the…

We report on the discovery of J0644+3344, a bright deeply eclipsing cataclysmic variable (CV) binary. Spectral signatures of both binary components and an accretion disk can be seen at optical wavelengths. The optical spectrum shows broad H…

天体物理学 · 物理学 2009-11-13 D. K. Sing , E. M. Green , S. B. Howell , J. B. Holberg , M. Lopez-Morales , J. S. Shaw , G. D. Schmidt

We present mid-IR observations of the Galactic Luminous Blue Variable (LBV) HR Car and its associated nebula carried out with the Spitzer Space Telescope using both IRAC and IRS, as part of a GTO program aimed to study stellar ejecta from…

星系天体物理 · 物理学 2011-02-11 G. Umana , C. S. Buemi , C. Trigilio , J. L. Hora , G. G. Fazio , P. Leto

Aims. We aim to determine the redshift (or stringent lower limits) of a number of bright BL Lacs objects. Methods. We secured medium resolution optical and near-infrared spectra of 4 bright BL Lac objects of unknown redshift using the…

星系天体物理 · 物理学 2014-11-05 Marco Landoni , Renato Falomo , Aldo Treves , Boris Sbarufatti

We have detected three new x-ray point sources, in addition to the known low-mass x-ray binary (LMXB) X1832-330, in the globular cluster NGC 6652 with a Chandra 1.6 ksec HRC-I exposure. Star 49 (M_{V}~4.7), suggested by Deutsch et al.(1998)…

天体物理学 · 物理学 2009-11-06 C. O. Heinke , P. D. Edmonds , J. E. Grindlay

We present a search and analysis of variable stars in the recently discovered Crater~II dwarf galaxy. Based on $B$, $V$, $I$ data collected with the Isaac Newton Telescope (FoV$\sim$0.44 square degrees) we detected 37 variable stars, of…

New B, V, I photometry was obtained for a sample of 152 variables (125 RR Lyrae's, 4 anomalous Cepheids, 11 classical Cepheids, 11 eclipsing binaries and a delta Scuti star) in two regions near the bar of the Large Magellanic Cloud (LMC).…

天体物理学 · 物理学 2007-05-23 M. Maio , G. Clementini , A. Bragaglia , E. Carretta , R. Gratton , L. Di Fabrizio

To better understand the LBV phenomenon, we analyze multi-epoch and multi-wavelength spectra and photometry of R71. Pre-outburst spectra are analyzed with the radiative transfer code CMFGEN to determine the star's fundamental stellar…

太阳与恒星天体物理 · 物理学 2017-12-20 A. Mehner , D. Baade , J. H. Groh , T. Rivinius , F. -J. Hambsch , E. S. Bartlett , D. Asmus , C. Agliozzo , T. Szeifert , O. Stahl