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Composite spectra Paper 16: HR 3222, a 2.5-yr binary with a metallic-line secondary

Monthly notices of the Royal Astronomical Society, 2010-03, Vol.402 (3), p.1675-1684

2010

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Composite spectra Paper 15: HD 216572, a triple system containing a short-period, double-lined secondary

Monthly notices of the Royal Astronomical Society, 2009-04, Vol.394 (3), p.1393-1408

2009

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A Spectroscopic Classification Survey to Search for New ρ Puppis Stars

The Astronomical journal, 2020-07, Vol.160 (1), p.52

2020

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Measurements of historical total ozone from the Chalonge-Divan stellar spectrum program: A reanalysis of the 1953–1972 data and a comparison with simultaneous Dobson Arosa measurements

Journal of Geophysical Research - Atmospheres, 2006-06, Vol.111 (D12), p.D12309-n/a

2006

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The double-lined spectroscopic binary HR 6046

Monthly notices of the Royal Astronomical Society, 2007-04, Vol.376 (4), p.1671-1679

2007

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Composite Spectra, Paper XXII HD 193349/50: a 3‐year binary whose apparently single hot secondary could itself be a former binary that is now merged

Astronomische Nachrichten, 2018-08, Vol.339 (7-8), p.586-595

2018

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HD 26367: A Nearby, Newly Identified Barium Dwarf

The Astronomical journal, 2007-07, Vol.134 (1), p.96-101, Article 96

2007

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Orbitally modulated photoexcited Si i emission in the eclipsing composite-spectrum binary ζ Aurigae

Monthly notices of the Royal Astronomical Society, 2016-02, Vol.456 (2), p.1346-1358

2016

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Dobson total ozone series of Oxford: Reevaluation and applications

Journal of Geophysical Research - Atmospheres, 2007-10, Vol.112 (D20), p.D20116-n/a

2007

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Composite Spectra, Paper XXI: 14 Serpentis

Astronomische Nachrichten, 2017-06, Vol.338 (5), p.604-613

2017

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First Direct Evidence That Barium Dwarfs Have White Dwarf Companions

The Astronomical journal, 2011-05, Vol.141 (5), p.160-jQuery1323897881848='48'

2011

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Composite spectra Paper 14: HR 1129, a long-period binary showing evidence of circumbinary material

Monthly notices of the Royal Astronomical Society, 2006-12, Vol.373 (4), p.1351-1368

2006

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Composite spectra: XX. 45 Cancri

Astronomische Nachrichten, 2015-03, Vol.336 (2), p.178-188

2015

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Detection and measurement of total ozone from stellar spectra: Paper 2. Historic data from 1935–1942

Atmospheric chemistry and physics, 2006, Vol.6 (8), p.2231-2240

Griffin, R. E. M.

2006

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Knowing What is Best

Proceedings of the International Astronomical Union, 2012-08, Vol.10 (H16), p.729-729

Griffin, R. E. M.

2012

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Binarity and Stellar Evolution

Proceedings of the International Astronomical Union, 2011-09, Vol.7 (S285), p.239-242

2011

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Composite spectra Paper 13: 93 Leonis, a chromospherically-active binary

Monthly notices of the Royal Astronomical Society, 2004-05, Vol.350 (2), p.685-706

2004

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A Spectroscopic Classification Survey to Search for New Puppis Stars

The Astronomical journal, 2020-07, Vol.160 (1)

2020

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The good, the bad and the really ugly: composite-spectrum binaries

Contributions of the Astronomical Observatory Skalnaté Pleso, 2020-01, Vol.50 (2)

Griffin, R.E.M.

2020

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Composite Spectra, Paper XXI: 14 Serpentis: An 8‐month binary whose hot component is a moderately rotating Am star

Astronomische Nachrichten, 2017-06, Vol.338 (5), p.604-613

2017

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The Effective Temperature of Arcturus

The Astronomical journal, 1999-06, Vol.117 (6), p.2998-3006

1999

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Orbitally modulated photoexcited Si?i emission in the eclipsing composite-spectrum binary [zeta] Aurigae

Monthly notices of the Royal Astronomical Society, 2016-02, Vol.456 (2), p.1346

2016

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Composite spectra Paper 16: HR 3222, a 2.5-yr binary with a metallic-line secondary

Monthly notices of the Royal Astronomical Society, 2010-03, Vol.402 (3), p.1675-1684

2010

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Composite spectra XIX: HD 208253, a long-period binary whose hot secondary has enhanced strontium and barium

Astronomische Nachrichten, 2013-08, Vol.334 (7), p.661-672

2013

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Composite spectra Paper 15: HD 216572, a triple system containing a short-period, double-lined secondary

Monthly notices of the Royal Astronomical Society, 2009-04, Vol.394 (3), p.1393-1408

2009

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Composite spectra Paper 16: HR 3222, a 2.5-yr binary with a metallic-line secondary

Composite spectra Paper 15: HD 216572, a triple system containing a short-period, double-lined secondary

A Spectroscopic Classification Survey to Search for New ρ Puppis Stars

Measurements of historical total ozone from the Chalonge-Divan stellar spectrum program: A reanalysis of the 1953–1972 data and a comparison with simultaneous Dobson Arosa measurements

The double-lined spectroscopic binary HR 6046

Composite Spectra, Paper XXII HD 193349/50: a 3‐year binary whose apparently single hot secondary could itself be a former binary that is now merged

HD 26367: A Nearby, Newly Identified Barium Dwarf

Orbitally modulated photoexcited Si i emission in the eclipsing composite-spectrum binary ζ Aurigae

Dobson total ozone series of Oxford: Reevaluation and applications

Composite Spectra, Paper XXI: 14 Serpentis

First Direct Evidence That Barium Dwarfs Have White Dwarf Companions

Composite spectra Paper 14: HR 1129, a long-period binary showing evidence of circumbinary material

Composite spectra: XX. 45 Cancri

Detection and measurement of total ozone from stellar spectra: Paper 2. Historic data from 1935–1942

Knowing What is Best

Binarity and Stellar Evolution

Composite spectra Paper 13: 93 Leonis, a chromospherically-active binary

A Spectroscopic Classification Survey to Search for New Puppis Stars

The good, the bad and the really ugly: composite-spectrum binaries

Composite Spectra, Paper XXI: 14 Serpentis: An 8‐month binary whose hot component is a moderately rotating Am star

The Effective Temperature of Arcturus

Orbitally modulated photoexcited Si?i emission in the eclipsing composite-spectrum binary [zeta] Aurigae

Composite spectra Paper 16: HR 3222, a 2.5-yr binary with a metallic-line secondary

Composite spectra XIX: HD 208253, a long-period binary whose hot secondary has enhanced strontium and barium

Composite spectra Paper 15: HD 216572, a triple system containing a short-period, double-lined secondary

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