Add to ORKGWe have studied white dwarfs in common proper motion pairs (CPMPs) to improve the semi-empirical initial–final mass relationship of white dwarfs. In this contribution, we re- port new results obtained from spectroscopic observations of both members of several CPMPs composed of a F, G or K type star and a DA white dwarf.Peer Reviewe
Thesis submitted for the degree of Master of Philosophy, Macquarie University, Department of Physics...
Using the most recent results about white dwarfs (WDs) in ten open clusters, we revisit semiempirica...
<p>We present samples from our posterior distribution of initial-final mass relations implied by our...
Context.The initial-final mass relationship of white dwarfs, which is poorly constrained, is of para...
A promising approach to decrease the uncertainties in the initial-final mass relationship, which is ...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
In this contribution we revisit the initial-final mass relationship of white dwarfs, which links the...
Intermediate mass stars either end their lives as a white dwarf (WD) or a neutron star, depending al...
Recent studies of white dwarfs in open clusters have provided new constraints on the initial-final m...
We present the mass distribution, gravitational redshifts, radial velocities, and space motions of w...
The initial-final mass relationship connects the mass of a white dwarf with the mass of its progenit...
The initial final mass relationship of white dwarfs is the function that relates the mass of the whi...
We present the initial–final mass relation derived from 10 white dwarfs in wide binaries that consis...
We use data from Gaia’s second data release (DR2) to constrain the initial-final mass relation (IFMR...
Thesis submitted for the degree of Master of Philosophy, Macquarie University, Department of Physics...
Using the most recent results about white dwarfs (WDs) in ten open clusters, we revisit semiempirica...
<p>We present samples from our posterior distribution of initial-final mass relations implied by our...
Context.The initial-final mass relationship of white dwarfs, which is poorly constrained, is of para...
A promising approach to decrease the uncertainties in the initial-final mass relationship, which is ...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
Context. The initial-final mass relationship of white dwarfs, which is poorly constrained, is of par...
In this contribution we revisit the initial-final mass relationship of white dwarfs, which links the...
Intermediate mass stars either end their lives as a white dwarf (WD) or a neutron star, depending al...
Recent studies of white dwarfs in open clusters have provided new constraints on the initial-final m...
We present the mass distribution, gravitational redshifts, radial velocities, and space motions of w...
The initial-final mass relationship connects the mass of a white dwarf with the mass of its progenit...
The initial final mass relationship of white dwarfs is the function that relates the mass of the whi...
We present the initial–final mass relation derived from 10 white dwarfs in wide binaries that consis...
We use data from Gaia’s second data release (DR2) to constrain the initial-final mass relation (IFMR...
Thesis submitted for the degree of Master of Philosophy, Macquarie University, Department of Physics...
Using the most recent results about white dwarfs (WDs) in ten open clusters, we revisit semiempirica...
<p>We present samples from our posterior distribution of initial-final mass relations implied by our...