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相关论文: Two Luminous Post-AGB Stars in the Galactic Globul…

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We present new H-band echelle spectra, obtained with the NIRSPEC spectrograph at Keck II, for the massive star cluster "B" in the nearby dwarf irregular galaxy NGC 1569. From spectral synthesis and equivalent width measurements we obtain…

天体物理学 · 物理学 2009-11-13 S. S. Larsen , L. Origlia , J. P. Brodie , J. S. Gallagher

This paper presents the first census of Galactic post-Asymptotic Giant Branch stars in the HR diagram. We combined Gaia DR3 parallax-based distances with extinction corrected integrated fluxes, and derived luminosities for a sample of 185…

太阳与恒星天体物理 · 物理学 2022-08-17 René D. Oudmaijer , Emma R. M. Jones , Miguel Vioque

We present the results of a photometric study of the early-type galaxy NGC 6876 and the surrounding globular cluster system (GCS). The host galaxy is a massive elliptical, the brightest of this type in the Pavo Group. According to its…

星系天体物理 · 物理学 2019-07-05 Ana Inés Ennis , Lilia Patricia Bassino , Juan Pablo Caso , Bruno Javier De Bórtoli

Recent observations have shown that a growing number of the most massive Galactic globular clusters contain multiple populations of stars with different [Fe/H] and neutron-capture element abundances. NGC 6273 has only recently been…

(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

We analyse 8 years of PASS 8 Fermi-LAT data, in the 60 MeV - 300 GeV energy range, from 30 high Galactic latitude globular clusters. Six of these globular clusters are detected with a TS > 25, with NGC 6254 being detected as gamma-ray…

高能天体物理现象 · 物理学 2018-08-15 Sheridan J. Lloyd , Paula M. Chadwick , Anthony M. Brown

The massive cluster of galaxies Abell 2219 (z = 0.228) was observed at 14.3 $\mu$m with the Infrared Space Observatory and results were published by Barvainis et al. (1999). These observations have been reanalyzed using a method…

The Galactic Center region, including the nuclear disk, has until recently been largely avoided in chemical census studies because of extreme extinction and stellar crowding. Making use of the latest APOGEE data release (DR16), we are able…

We present the results of spectroscopy and CCD photometry of the intermediate-luminosity red transient PSN J13100734+3410514 in the galaxy UGC 8246 performed in February and June 2014 with the Russian 6-meter telescope and SCORPIO spectral…

太阳与恒星天体物理 · 物理学 2014-12-23 E. A. Barsukova , V. P. Goranskij , A. F. Valeev , S. S. Kaisin

To investigate the asymptotic giant branch (AGB) population in the Galactic halo, we search for pulsating AGB stars at a heliocentric distance over 50kpc. Our research is based on the Catalina Southern Survey (CSS) catalogue of variables,…

星系天体物理 · 物理学 2021-06-30 Nicolas Mauron , Kamo S. Gigoyan , Tim R. Kendall , Kelly M. Hambleton

J, H, and K' images are used to investigate the asymptotic giant branch (AGB) content of the Local Group dwarf elliptical galaxy NGC 205. The AGB on the (K, H-K) and (K, J-K) color-magnitude diagrams consists of two sequences: a…

天体物理学 · 物理学 2009-11-10 T. J. Davidge

We present a spectral analysis of the UV-bright star Y453 in M4. Model fits to the star's optical spectrum yield T_eff ~ 56,000 K. Fits to the star's FUV spectrum, obtained with the Cosmic Origins Spectrograph (COS) on board the Hubble…

太阳与恒星天体物理 · 物理学 2017-09-06 William V. Dixon , Pierre Chayer , Marilyn Latour , Marcelo Miguel Miller Bertolami , Robert A. Benjamin

We present observations of the center of the Galactic globular cluster NGC 6273, obtained with the HST/WFPC2 camera as part of the snapshot program GO-7470. A B, V color-magnitude diagram (CMD) for ~28,000 stars is presented and discussed.…

天体物理学 · 物理学 2009-10-31 G. Piotto , M. Zoccali , I. R. King , S. G. Djorgovski C. Sosin , R. M. Rich , G. Meylan

The evolutionary status of 24 post-AGB stars is presented based on Gaia DR3 data. All 24 stars have parallaxes accurate to better than 3 X sigma and have RUWE values less than 1.4. Based on the Gaia DR3 distances the absolute luminosities…

太阳与恒星天体物理 · 物理学 2022-10-04 M. Parthasarathy , Marina. Kounkel , Keivan G. Stassun

We present the discovery and characterisation of the post-common-envelope central star system in the planetary nebula PN G283.7$-$05.1. Deep images taken as part of the POPIPlaN survey indicate that the nebula may possess a bipolar…

We present evidence that some of the compact, luminous, young star clusters recently discovered through images taken with the Hubble Space Telescope (HST) have masses comparable to those of old Galactic globular clusters. The "super star…

天体物理学 · 物理学 2009-10-28 Luis C. Ho , Alexei V. Filippenko

The core of the galactic globular cluster M13 (NGC 6205) has been observed with WFPC2 on the Hubble Space Telescope through visual, blue and mid- and far-UV filters in a programme devoted to study the UV population in a sample of Galactic…

天体物理学 · 物理学 2016-01-13 Francesco R. Ferraro , Barbara Paltrinieri , Flavio Fusi Pecci , Robert T. Rood , Ben Dorman

We report on HST/WFPC2 U,V and far-ultraviolet observations of two Galactic Globular Clusters (GGCs), NGC 6205 = M13 and NGC 6093 = M80. Both of these clusters have horizontal-branch (HB) tails that extend to the helium-burning main…

天体物理学 · 物理学 2009-10-30 Francesco R. Ferraro , Barbara Paltrinieri , Flavio Fusi Pecci , Ben Dorman , Robert T. Rood

We present a complete study of the morphology of post-Asymptotic Giant Branch (AGB) stars. Post-AGB is a very short evolutionary phase between the end of the AGB and the beginning of the Planetary Nebula (PN) stage (between 100 and 10,000…

太阳与恒星天体物理 · 物理学 2015-05-28 A. Manchado , D. A. Garcia-Hernandez , E. Villaver , J. Guironnet de Massas

We report the discovery using Hubble Space Telescope imaging and Keck spectroscopy of a very bright, highly magnified (~30*) Lyman Break Galaxy (LBG) at z=3.07 in the field of the massive z=0.33 cluster MACSJ2135.2-0102. The system…