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相关论文: Study of UV bright stellar populations in the glob…

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We present the results obtained from the UV photometry of the globular cluster NGC 1261 using Far-UV (FUV) and Near-UV (NUV) images acquired with the Ultraviolet Imaging Telescope (UVIT) onboard the Astrosat satellite. We utilized the UVIT…

太阳与恒星天体物理 · 物理学 2020-12-23 Sharmila Rani , Gajendra Pandey , Annapurni Subramaniam , Snehalala Sahu , N. Kameswara Rao

We present the far-UV (FUV) photometry of images acquired with UVIT on AstroSat to probe the horizontal branch (HB) population of the Galactic globular cluster NGC 2298. UV-optical color-magnitude diagrams (CMDs) are constructed for member…

太阳与恒星天体物理 · 物理学 2022-01-05 Sharmila Rani , Gajendra Pandey , Annapurni Subramaniam , Chul Chung , Snehalata Sahu , N. Kameswara Rao

We present detailed photometric observations of the Galactic globular cluster NGC 7492 using the data obtained with two far-ultraviolet (FUV: 1300 - 1800 \AA) and three near-ultraviolet (NUV: 2000 - 3000 \AA) filters of Ultraviolet Imaging…

We present the UV photometry of the globular cluster NGC 1851 using images acquired with the Ultra-violet Imaging Telescope (UVIT) onboard the ASTROSAT satellite. PSF-fitting photometric data derived from images in two far-UV (FUV) filters…

We present far ultraviolet (FUV) observations of globular cluster NGC 4147 using three FUV filters, BaF2 (F154W), Sapphire (F169M), and Silica (F172M) of Ultra-Violet Imaging Telescope (UVIT) on-board the \mbox{{\em AstroSat}} satellite. We…

Globular clusters being old and densely packed serve as ideal laboratories to test stellar evolution theories. Although there is enormous literature on globular clusters in optical bands, studies in the ultraviolet (UV) regime are sparse.…

星系天体物理 · 物理学 2022-06-15 K. J. Nikitha , S. Vig , S. K. Ghosh

We present a study of Far Ultraviolet (FUV) bright horizontal branch (HB) stars to understand the peculiarities seen in the HB sequence of the Globular Cluster NGC 1851, using ground and space based multi-wavelength data. Optical and UV…

太阳与恒星天体物理 · 物理学 2020-12-16 Gaurav Singh , Snehalata Sahu , Annapurni Subramaniam , R. K. S. Yadav

We have studied ultraviolet (UV) bright sources in the Galactic globular cluster (GGC) NGC 4590 using Ultraviolet Imaging Telescope (UVIT) on-board the \mbox{{\em AstroSat}} satellite. Using UV-optical color-magnitude diagrams (CMDs), we…

In this study, we identified and characterized the hot and luminous UV-bright stars in the globular cluster NGC 2808. We combined data from the Ultra Violet Imaging Telescope (UVIT) on-board the Indian space satellite, AstroSat, with the…

太阳与恒星天体物理 · 物理学 2021-02-24 Deepthi S. Prabhu , Annapurni Subramaniam , Snehalata Sahu

A recent study of hot (20,000 to 30,000 K) extreme horizontal branch (EHB) stars in globular clusters (GCs) has led to the discovery of their variability. It is suggested that this variability is driven by the projected rotation of magnetic…

太阳与恒星天体物理 · 物理学 2021-09-15 Deepthi S. Prabhu , Annapurni Subramaniam , Snehalata Sahu

We present stellar photometry in the UBV passbands for the globular cluster M5 = NGC5904. The observations, short-exposured photographic plates and CCD frames, were obtained in the RC-focus of the 2m telescope of the Natl. Astron. Obs.…

天体物理学 · 物理学 2009-11-06 Haralambi Markov , Nedka Spassova , Plamen Baev

We present the UV photometry of the old open cluster NGC188 obtained using images acquired with Ultraviolet Imaging Telescope (UVIT) on board the ASTROSAT satellite, in two far-UV (FUV) and one near-UV (NUV) filters. UVIT data is utilised…

太阳与恒星天体物理 · 物理学 2021-06-23 Sharmila Rani , Annapurni Subramaniam , Sindhu Pandey , Snehalata Sahu , Chayan Mondal , Gajendra Pandey

A complete census of Blue Horizontal Branch (BHB) and Blue Straggler Star (BSS) population within the 10$'$ radius from the center of the Globular Cluster, NGC 288 is presented, based on the images from the Ultraviolet Imaging Telescope…

太阳与恒星天体物理 · 物理学 2018-10-04 Snehalata Sahu , Annapurni Subramaniam , Patrick Côté , N. Kameswara Rao , Peter B. Stetson

As part of a large project aimed at characterizing the ultraviolet (UV) properties of globular clusters, we present here a theoretical and observational analysis aimed at setting the framework for the determination of horizontal branch (HB)…

太阳与恒星天体物理 · 物理学 2015-06-23 E. P. Lagioia , E. Dalessandro , F. R. Ferraro , M. Salaris , B. Lanzoni , A. Pietrinferni , S. Cassisi

(Abriged)This work studies in more detail the stellar population, including its photometric properties and characteristics, in the rarely studied southern Galactic globular cluster NGC 1261. We focus on the brighter sequences of the…

星系天体物理 · 物理学 2015-05-18 V. Kravtsov , G. Alcaino , G. Marconi , F. Alvarado

Globular clusters represent stellar laboratories where observations can be used to validate models of stellar evolution. In this study, we put forth new ultraviolet (UV) photometric results of stars in the Galactic globular cluster NGC…

太阳与恒星天体物理 · 物理学 2019-03-06 Rashi Jain , S. Vig , S. K. Ghosh

We have obtained medium-resolution spectra of seven UV-bright stars discovered on images of four southern globular clusters obtained with the Ultraviolet Imaging Telescope (UIT). Effective temperatures, surface gravities and helium…

天体物理学 · 物理学 2007-05-23 S. Moehler , W. Landsman , R. Napiwotzki

We used the Ultraviolet Imaging Telescope during the March 1995 Astro-2 mission to obtain a deep far-UV image of the globular cluster NGC 362, which was formerly thought to have an almost entirely red horizontal branch (HB). 84 hot (T_eff >…

We present a 1620 A image of the nearby globular cluster NGC 6752 obtained with the Ultraviolet Imaging Telescope (UIT) during the Astro-2 mission of the Space Shuttle Endeavour in 1995 March. An ultraviolet-visible color-magnitude diagram…

Relying on U,B imagery at the Italian Telescopio Nazionale Galileo (TNG), we report here the discovery of a sample of 13 new UV-bright post-HB candidate stars in the field of the galactic open cluster NGC 6791. Owing to its super-solar…

天体物理学 · 物理学 2016-08-30 L. M. Buson , E. Bertone , A. Buzzoni , G. Carraro
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