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相关论文: Halo White Dwarfs, Thick Disks and a Sanity Check

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The interpretation of the old, cool white dwarfs recently found by Oppenheimer et al. (2001) is still controversial. Whereas these authors claim that they have finally found the elusive ancient halo white dwarf population that contributes…

天体物理学 · 物理学 2009-11-07 Santiago Torres , Enrique Garcia-Berro , Andreas Burkert , Jordi Isern

We present an alternative interpretation of the nature of the extremely cool, high-velocity white dwarfs identified by Oppenheimer et al (2001) in a high-latitude astrometric survey. We argue that the velocity distribution of the majority…

天体物理学 · 物理学 2009-11-06 I. Neill Reid , Kailash C. Sahu , Suzanne L. Hawley

The interpretation of high proper motion white dwarfs detected by Oppenheimer et al (2001) was the start of a lively controversy. While the discoverers identify a large fraction of their findings as dark halo members, others interpret the…

天体物理学 · 物理学 2009-11-07 Celine Reyle , Annie C. Robin , Michel Creze

We analyse the kinematics of the entire spectroscopic sample of 99 recently discovered high proper-motion white dwarfs by Oppenheimer et al. using a maximum-likelihood analysis, and discuss the claim that the high-velocity white dwarfs are…

天体物理学 · 物理学 2007-05-23 L. V. E. Koopmans , R. D. Blandford

Based on a proper motion survey, Oppenheimer et al. claim the detection of a white dwarf component of the dark matter of the halo. I show that most of the white dwarfs in their sample are likely disk white dwarfs which have been previously…

天体物理学 · 物理学 2007-05-23 David S. Graff

We examine the claim by Oppenheimer et al. (2001) that the local halo density of white dwarfs is an order of magnitude higher than previously thought. As it stands, the observational data support the presence of a kinematically distinct…

天体物理学 · 物理学 2017-08-23 L. V. E. Koopmans , R. D. Blandford

We discuss the recent discovery by Oppenheimer et al (2001) of old, cool white dwarf stars, which may be the first direct detection of Galactic halo dark matter. We argue here that the contribution of more mundane white dwarfs of the…

天体物理学 · 物理学 2009-11-07 Chris Flynn , Janne Holopainen , Johan Holmberg

A detailed analysis of halo white dwarf candidates is presented, which is based on model atmosphere fits to observed energy distributions built from photoelectric or photographic magnitudes. Most of the candidates identified in reduced…

天体物理学 · 物理学 2009-11-07 P. Bergeron

We present a detailed analysis of the white dwarf luminosity functions derived from the local 40 pc sample and the deep proper motion catalog of Munn et al (2014, 2017). Many of the previous studies ignored the contribution of thick disk…

Oppenheimer et al. (2001) have argued recently that at least 2% of the Galactic halo is comprised of white dwarfs If true, this finding has crucial implications for understanding the formation and evolution of the Milky Way. We draw…

天体物理学 · 物理学 2007-05-23 Brad K. Gibson , Chris Flynn

A detailed analysis of 32 of the 38 halo white dwarf candidates identified by Oppenheimer et al. is presented, based on model atmosphere fits to observed energy distributions built from optical BVRI and infrared JHK CCD photometry.…

天体物理学 · 物理学 2009-11-10 P. Bergeron , Maria Teresa Ruiz , M. Hamuy , S. K. Leggett , M. J. Currie , C. -P. Lajoie , P. Dufour

The contribution of white dwarfs of the different Galactic populations to the stellar content of our Galaxy is only poorly known. Some authors claim a vast population of halo white dwarfs, which would be in accordance with some…

太阳与恒星天体物理 · 物理学 2009-07-22 Ralf Napiwotzki

We present the discovery and spectroscopic identification of two very high proper motion ancient white dwarf stars, found in a systematic proper motion survey. Their kinematics and apparent magnitude clearly indicate that they are halo…

天体物理学 · 物理学 2009-10-31 Rodrigo Ibata , Michael Irwin , Olivier Bienayme , Ralf Scholz , Jean Guibert

Recent observations suggest the existence of a white dwarf population in the Galactic halo, while others suggest that deuterium has been astrated in systems at high redshift and low metallicity. We propose that these observations could be…

天体物理学 · 物理学 2009-09-15 Brian D. Fields , Keith A. Olive , Joseph Silk , Michel Casse , Elisabeth Vangioni-Flam

Oxygen and carbon are important elements in stellar populations. Their behavior refers to the formation history of the stellar populations. C and O abundances would also obviously influence stellar opacities and the overall metal abundance…

太阳与恒星天体物理 · 物理学 2016-12-21 Z. S. Ge , S. L. Bi , Y. Q. Chen , T. D. Li , J. K. Zhao , K. Liu , Fergusion J. W. , Y. Q. Wu

We present an alternative method for the kinematic analysis of high proper motion surveys and discuss its application to the survey of Oppenheimer et al. (2001) for the selection of reliable halo white dwarfs (WDs). The local WD space…

天体物理学 · 物理学 2009-11-10 A. Spagna , D. Carollo , M. G. Lattanzi , B. Bucciarelli

We have performed a search for halo white dwarfs as high proper motion objects in a second epoch WFPC2 image of the Groth-Westphal strip. We identify 24 high proper motion objects with mu > 0.014 ''/yr. Five of these high proper motion…

天体物理学 · 物理学 2009-11-07 Cailin A. Nelson , Kem H. Cook , Tim S. Axelrod , Jeremy R. Mould , Charles Alcock

Thanks to the recent space-borne mission Gaia, there is a nearly complete sample of white dwarfs up to about 100 parsecs from the Sun, which may have very diverse origins. We aim to compute the Galactic orbits for white dwarfs observed in…

太阳与恒星天体物理 · 物理学 2024-07-24 Ainhoa Zubiaur , Roberto Raddi , Santiago Torres

The Milky Way Galaxy contains a large, spherical component which is believed to harbor a substantial amount of unseen matter. Recent observations indirectly suggest that as much as half of this ``dark matter'' may be in the form of old,…

天体物理学 · 物理学 2009-10-12 B. R. Oppenheimer , N. C. Hambly , A. P. Digby , S. T. Hodgkin , D. Saumon

We present new evidence, based on faint HST proper-motions, for a bi-modal kinematic population of old white dwarfs, representative of the Thick-Disk and Halo of our Galaxy. This evidence supports the idea of a massive Halo comprised of…

天体物理学 · 物理学 2009-11-07 Rene A. Mendez
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