-
1
-
2
Search for Sub-Solar Mass Binaries with Einstein Telescope and Cosmic Explorer
Published 2022-02-01“…A possible detection of sub-solar mass ultra-compact objects would lead to new perspectives on the existence of black holes that are not of astrophysical origin and/or pertain to formation scenarios of exotic ultra-compact objects. …”
Get full text
Article -
3
The Hidden Companion in J1527: A 0.69 Solar-mass White Dwarf?
Published 2024-01-01Get full text
Article -
4
GW170608: Observation of a 19 Solar-mass Binary Black Hole Coalescence
Published 2018Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
5
A 1.9 solar-mass neutron star candidate in a 2-year orbit
Published 2024-04-01Get full text
Article -
6
The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3.
Published 2013“…Although the mean molecular gas mass (5 × 10(10) solar masses) of the submillimetre bright galaxies can explain the formation of typical elliptical galaxies, it is inadequate to form elliptical galaxies that already have stellar masses above 2 × 10(11) solar masses at z ≈ 2. …”
Journal article -
7
The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3
Published 2013“…Although the mean molecular gas mass (5 × 10 10 solar masses) of the submillimetre bright galaxies can explain the formation of typical elliptical galaxies, it is inadequate to form elliptical galaxies that already have stellar masses above 2 × 10 11 solar masses at z ≈ 2. …”
Journal article -
8
GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence
Published 2016Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
9
GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
Published 2017Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Get full text
Article -
10
An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5
Published 2021“…This quasar has a bolometric luminosity of 4 × 10 13 times the luminosity of the Sun and a black-hole mass of 8 × 10 8 solar masses. The existence of this supermassive black hole when the Universe was only 690 million years old-just five per cent of its current age-reinforces models of early black-hole growth that allow black holes with initial masses of more than about 10 4 solar masses or episodic hyper-Eddington accretion. …”
Get full text
Article -
11
An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5
Published 2022“…This quasar has a bolometric luminosity of 4 × 10 13 times the luminosity of the Sun and a black-hole mass of 8 × 10 8 solar masses. The existence of this supermassive black hole when the Universe was only 690 million years old-just five per cent of its current age-reinforces models of early black-hole growth that allow black holes with initial masses of more than about 10 4 solar masses or episodic hyper-Eddington accretion. …”
Get full text
Article -
12
The Orbit and Mass of the Sagittarius Dwarf Galaxy
Published 1999“…At one extreme the Dwarf initially possesses 10^{11} Solar Mass and starts from a Galactocentric distance 200 kpc. …”
Journal article -
13
The LMC Microlensing Events: Evidence for a Warped and Flaring Milky Way Disk?
Published 1997“…A normal stellar population of 0.5 solar mass stars should be visible. The other obvious candidate for the lenses is a population of white dwarfs. …”
Journal article -
14
Mathematical model for the 0.5 billion years aged Sun
Published 2000-01-01“…An algorithm is given for constructing evolutionary tracks for a star with the mass equal to one solar mass. The presented model can be applied to the stars belonging to the inferior main sequence, which have the proton-proton reaction as energy source and present a radiative core and a convective shell. …”
Get full text
Article -
15
The origin of the Earth - What's new?
Published 2006“…At the present time we do not know whether our solar system, with terrestrial planets located within a few astronomical units2 of a solar-mass star, is unusual or common. Neither do we understand where the water that made Earth habitable came from, nor whether life in the Universe is rare or plentiful. …”
Journal article -
16
Molecular richness in protostars: Lessons learnt from spectral observations
Published 2022-01-01“…The present contribution summarises what we have learnt, in the past decade or so, about the molecular contents in solar-mass protostellar sources, and suggests a few guidelines to stimulate progress in the field.…”
Get full text
Article -
17
Stiff phases in strongly coupled gauge theories with holographic duals
Published 2017-11-01“…This has important consequences in particular for the physics of compact stars, where the detection of two solar mass neutron stars has been shown to require very stiff equations of state. …”
Get full text
Article -
18
Weaker yet again: mass spectrum-consistent cosmological constraints on the neutrino lifetime
Published 2022-07-01“…We find that for a parent neutrino of mass $$m_{\nu H} \lesssim 0.1$$ m ν H ≲ 0.1 eV, the new phase space factor weakens the constraint on its lifetime by up to a factor of 50 if $$\varDelta m_\nu ^2$$ Δ m ν 2 corresponds to the atmospheric mass gap and up to $$10^{5}$$ 10 5 if the solar mass gap, in comparison with naïve estimates that assume $$m_{\nu l}=0$$ m ν l = 0 . …”
Get full text
Article -
19
Searching for isovector signatures in the neutron-rich oxygen and calcium isotopes
Published 2015-09-01“…This same model—labeled “FSUGarnet”—predicts R1.4=(13.0±0.1) km for the radius of a “canonical” 1.4M⊙ neutron star, yet is also able to support a two-solar-mass neutron star.…”
Get full text
Article -
20
Probing first-order electroweak phase transition via primordial black holes in the effective field theory
Published 2023-03-01“…Since the mass of such primordial black holes is evaluated to be about 10−5 of the solar mass, current and future microlensing observations such as Subaru HSC, OGLE, PRIME and Roman Space Telescope may be able to probe the electroweak phase transition. …”
Get full text
Article