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Another Independent Discovery of the 1946 Eruption of the Recurrent Nova T Coronae Borealis

Research notes of the AAS, 2024-09, Vol.8 (9), p.233

Shears, J. H.

2024

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CO Fundamental and First Overtone Emission in the Nova V496 Scuti

Research notes of the AAS, 2023-08, Vol.7 (8), p.185

2023

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Emission Line Profile Variations in the Early Coronal Phase of the Nova V2944 Ophiuchi

Research notes of the AAS, 2023-04, Vol.7 (4), p.64

2023

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Discovery of 13 New Orbital Periods for Classical Novae

Research notes of the AAS, 2021-06, Vol.5 (6), p.150

Schaefer, Bradley E.

2021

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X-Ray Emissions from Accreting White Dwarfs: A Review

Publications of the Astronomical Society of the Pacific, 2017-06, Vol.129 (976), p.62001

Mukai, K.

2017

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Evidence for Multiple Shocks from the γ-Ray Emission of RS Ophiuchi

The Astrophysical journal, 2023-04, Vol.947 (2), p.70

2023

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Testing the disk instability model of cataclysmic variables

Astronomy and astrophysics (Berlin), 2018-09, Vol.617, p.A26

2018

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POPULATION SYNTHESIS OF CATACLYSMIC VARIABLES. I. INCLUSION OF DETAILED NUCLEAR EVOLUTION

The Astrophysical journal, 2015-08, Vol.809 (1), p.1-19

2015

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Evolutionary Period Changes for 52 Cataclysmic Variables, and the Failure for the Most-fundamental Prediction of the Magnetic Braking Model

The Astrophysical journal, 2024-05, Vol.966 (2), p.155

Schaefer, Bradley E.

2024

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Post-outburst and Nebular Phase Spectra of the Fe ii-type Nova V378 Serpentis

Research notes of the AAS, 2024-10, Vol.8 (10), p.275

2024

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The Remarkable Spin-down and Ultrafast Outflows of the Highly Pulsed Supersoft Source of Nova Herculis 2021

Astrophysical journal. Letters, 2021-12, Vol.922 (2), p.L42

2021

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A catalogue of over 10 million variable source candidates in ZTF Data Release 1

Monthly notices of the Royal Astronomical Society, 2020-11, Vol.499 (4), p.5782-5790

2020

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Introducing the Condor Array Telescope – III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell

Monthly notices of the Royal Astronomical Society, 2024-03, Vol.529 (1), p.212-223

2024

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New Method of Estimating Binary's Mass Ratios by Using Superhumps

Publications of the Astronomical Society of Japan, 2013-12, Vol.65 (6)

2013

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The Recurrent Nova V745 Sco had a Classical Nova Eruption in 1897 July

Research notes of the AAS, 2024-03, Vol.8 (3), p.93

Schaefer, Bradley E.

2024

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On Presolar Stardust Grains from CO Classical Novae

The Astrophysical journal, 2018-03, Vol.855 (2), p.76

2018

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When will the Next T CrB Eruption Occur?

Research notes of the AAS, 2024-10, Vol.8 (10), p.272

Schneider, Jean

2024

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Hydrodynamic Simulations of Oxygen–Neon Classical Novae as Galactic 7Li Producers and Potential Accretion-induced Collapse Progenitors We dedicate this paper to the memory of R. Mark Wagner. Friend, collaborator, exemplary observational astronomer, and contributor to studies of classical novae and transient objects for more than 40 years. He will be missed

The Astrophysical journal, 2024-02, Vol.962 (2)

2024

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1000 cataclysmic variables from the Catalina Real-time Transient Survey

Monthly notices of the Royal Astronomical Society, 2014-10, Vol.443 (4), p.3174-3207

2014

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The Masses and Accretion Rates of White Dwarfs in Classical and Recurrent Novae

The Astrophysical journal, 2018-06, Vol.860 (2), p.110

2018

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Early Spectral Evolution of Classical Novae: Consistent Evidence for Multiple Distinct Outflows

The Astrophysical journal, 2020-12, Vol.905 (1), p.62

2020

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A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae

The Astrophysical journal, 2017-04, Vol.839 (2), p.109

2017

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CO and C i Emission in the Early Spectrum of the Nova V1391 Cassiopeiae

Research notes of the AAS, 2024-03, Vol.8 (3), p.80

2024

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Binary Interaction Dominates Mass Ejection in Classical Novae

The Astrophysical journal, 2022-10, Vol.938 (1), p.31

2022

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Hydrodynamic Simulations of Oxygen–Neon Classical Novae as Galactic 7Li Producers and Potential Accretion-induced Collapse Progenitors

The Astrophysical journal, 2024-02, Vol.962 (2), p.191

2024

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Another Independent Discovery of the 1946 Eruption of the Recurrent Nova T Coronae Borealis

CO Fundamental and First Overtone Emission in the Nova V496 Scuti

Emission Line Profile Variations in the Early Coronal Phase of the Nova V2944 Ophiuchi

Discovery of 13 New Orbital Periods for Classical Novae

X-Ray Emissions from Accreting White Dwarfs: A Review

Evidence for Multiple Shocks from the γ-Ray Emission of RS Ophiuchi

Testing the disk instability model of cataclysmic variables

POPULATION SYNTHESIS OF CATACLYSMIC VARIABLES. I. INCLUSION OF DETAILED NUCLEAR EVOLUTION

Evolutionary Period Changes for 52 Cataclysmic Variables, and the Failure for the Most-fundamental Prediction of the Magnetic Braking Model

Post-outburst and Nebular Phase Spectra of the Fe ii-type Nova V378 Serpentis

The Remarkable Spin-down and Ultrafast Outflows of the Highly Pulsed Supersoft Source of Nova Herculis 2021

A catalogue of over 10 million variable source candidates in ZTF Data Release 1

Introducing the Condor Array Telescope – III. The expansion and age of the shell of the dwarf nova Z Camelopardalis, and detection of a second, larger shell

New Method of Estimating Binary's Mass Ratios by Using Superhumps

The Recurrent Nova V745 Sco had a Classical Nova Eruption in 1897 July

On Presolar Stardust Grains from CO Classical Novae

When will the Next T CrB Eruption Occur?

1000 cataclysmic variables from the Catalina Real-time Transient Survey

The Masses and Accretion Rates of White Dwarfs in Classical and Recurrent Novae

Early Spectral Evolution of Classical Novae: Consistent Evidence for Multiple Distinct Outflows

A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae

CO and C i Emission in the Early Spectrum of the Nova V1391 Cassiopeiae

Binary Interaction Dominates Mass Ejection in Classical Novae

Hydrodynamic Simulations of Oxygen–Neon Classical Novae as Galactic 7Li Producers and Potential Accretion-induced Collapse Progenitors

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