The Astrophysical Journal

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History

The journal was founded in 1895 by George Ellery Hale and James E. Keeler as The Astrophysical Journal: An International Review of Spectroscopy and Astronomical Physics. [9] In addition to the two founding editors, there was an international board of associate editors: M. A. Cornu, Paris; N. C. Dunér, Upsala; William Huggins, London; P. Tacchini, Rome; H. C. Vogel, Potsdam, C. S. Hastings, Yale; A. A. Michelson, Chicago; E. C. Pickering, Harvard; H. A. Rowland, Johns Hopkins; and C. A. Young, Princeton. [10] It was intended that the journal would fill the gap between journals in astronomy and physics, providing a venue for publication of articles on astronomical applications of the spectroscope; on laboratory research closely allied to astronomical physics, including wavelength determinations of metallic and gaseous spectra and experiments on radiation and absorption; on theories of the Sun, Moon, planets, comets, meteors, and nebulae; and on instrumentation for telescopes and laboratories. [10] The further development of ApJ up to 1995 was outlined by Helmut Abt in an article entitled "Some Statistical Highlights of the Astrophysical Journal" in 1995. [11]

Editors

The following persons have been editors-in-chief of the journal:

See also

Related Research Articles

<span class="mw-page-title-main">Subrahmanyan Chandrasekhar</span> Indian-American physicist (1910-1995)

Subrahmanyan Chandrasekhar was an Indian-American theoretical physicist who made significant contributions to the scientific knowledge about the structure of stars, stellar evolution and black holes. He was awarded the 1983 Nobel Prize in physics along with William A. Fowler for "...theoretical studies of the physical processes of importance to the structure and evolution of the stars". His mathematical treatment of stellar evolution yielded many of the current theoretical models of the later evolutionary stages of massive stars and black holes. Many concepts, institutions and inventions, including the Chandrasekhar limit and the Chandra X-Ray Observatory, are named after him.

<span class="mw-page-title-main">Gamma Trianguli Australis</span> Star in the constellation Triangulum Australe

Gamma Trianguli Australis, Latinized from γ Trianguli Australis, is a single, white-hued star in the southern constellation of Triangulum Australe. Along with Alpha and Beta Trianguli Australis it forms a prominent triangular asterism that gives the constellation its name. It is the third-brightest member of this constellation with an apparent visual magnitude of +2.87. Based upon parallax measurements, Gamma Trianguli Australis is located at a distance of about 190 light-years from Earth.

<span class="mw-page-title-main">109 Virginis</span> Star in the constellation Virgo

109 Virginis is a single, white-hued star in the zodiac constellation of Virgo, located some 134.5 light years away from the Sun. It is the seventh-brightest member of this constellation, having an apparent visual magnitude of +3.72.

<span class="mw-page-title-main">Xi Virginis</span> Star in the constellation Virgo

Xi Virginis is a solitary star in the zodiac constellation of Virgo. It is bright enough to be seen with the naked eye, having an apparent visual magnitude of 4.83. The distance to this star is about 122 light years, as determined from parallax readings.

<span class="mw-page-title-main">108 Aquarii</span> Star in the constellation Aquarius

108 Aquarii is a star in the equatorial constellation of Aquarius. 108 Aquarii is the Flamsteed designation, although it also bears the Bayer designation i3 Aquarii and the variable star designation ET Aquarii. It has an apparent visual magnitude of 5.194 and can be seen with the naked eye under suitably dark skies. Based upon an annual parallax shift of 10.23, the distance to this star is 319 light-years.

<span class="mw-page-title-main">15 Cancri</span> Star in the constellation Cancer

15 Cancri is an α2 CVn-type variable star in the zodiac constellation of Cancer, located around 980 light years away. It has the variable star designation BM Cancri ; 15 Cancri is the Flamsteed designation. This system is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of about 5.6. It is moving away from the Earth with a heliocentric radial velocity of 25 km/s.

16 Lyrae is a suspected astrometric binary star system in the constellation Lyra, located 126 light years away from the Sun based on parallax. It is visible to the naked eye as a dim, white-hued star with a combined apparent visual magnitude of 5.00. The system is moving further away from the Earth with a heliocentric radial velocity of +5 km/s. It is a suspected member of the Ursa Major Moving Group stream.

HD 191984 is a double star in the equatorial constellation of Aquila. As of 2011, the components have an angular separation of 2.52″ along a position angle of 205.7°.

HD 30453 is a binary star system in the northern constellation of Auriga. It is visible to the naked eye with an apparent visual magnitude of 5.86. The system is located at a distance of approximately 334 light years from the Sun based on parallax. It is drifting further away from the Sun with a radial velocity of 16.65 km/s.

HR 3082 is a double star in the northern circumpolar constellation of Camelopardalis. It is faintly visible to the naked eye with an apparent visual magnitude of 5.39. The system is moving closer to the Sun with a heliocentric radial velocity of +2.7 km/s. It is currently at a distance of around 341 light years, based upon an annual parallax shift of 9.57 mas.

<span class="mw-page-title-main">21 Vulpeculae</span> Star in the constellation Vulpecula

21 Vulpeculae is a single, white-hued star in the northern constellation of Vulpecula. Its distance can be estimated from the annual parallax shift of 10.4302±0.0696 mas, yielding a separation of 313 light years. The star is faintly visible to the naked eye at night, having an apparent visual magnitude of 5.19. It is moving further away with a heliocentric radial velocity of about +7 km/s, having come within 243 ly (74.53 pc) around 4.2 million years ago.

<span class="mw-page-title-main">45 Herculis</span> Star in the constellation Hercules

45 Herculis is a solitary variable star in the northern constellation Hercules. It has the Bayer designation l Herculis and the variable star designation V776 Herculis. The Flamsteed designation for this star comes from the publication Historia Coelestis Britannica by John Flamsteed. It is the 45th star in Flamsteed list of stars in the constellation Hercules, and is visible to the naked eye with a baseline apparent visual magnitude of 5.22. Parallax measurements show this star to be about 400 light-years away from the Solar System. It is moving closer to the Earth with a heliocentric radial velocity of −16 km/s.

38 Geminorum is a binary star system in the northern zodiac constellation of Gemini. It has the Bayer designation e Geminorum, while 38 Geminorum is the Flamsteed designation. This system is visible to the naked eye as a faint, white-hued point of light with an apparent visual magnitude of 4.71. The primary component is a magnitude 4.75 star, while the secondary is magnitude 7.80. The system is located about 98 light years away from the Sun based on parallax, and is drifting further away with a radial velocity of +16 km/s. It is a potential member of the Tucana–Horologium stellar kinematic group.

<span class="mw-page-title-main">Iota Delphini</span> A-type giant star in the constellation Delphinus

Iota Delphini is a star in the constellation Delphinus. It has an apparent magnitude of about 5.4, meaning that it is just barely visible to the naked eye. Based upon parallax measurements made by the Gaia spacecraft, this star is located at a distance of 196 light years.

<span class="mw-page-title-main">21 Persei</span> Star in the constellation Perseus

21 Persei is a single, variable star in the northern constellation of Perseus, located about 331 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.10 km/s. The object is moving further from the Earth with a heliocentric radial velocity of +8.5 km/s. It has the variable star designation LT Persei; 21 Persei is the Flamsteed designation.

Tau7 Eridani is a solitary star in the constellation Eridanus. It is visible to the naked eye with an apparent visual magnitude of 5.235. Using the parallax method, the distance to this star can be estimated as around 251 light years.

<span class="mw-page-title-main">1 Delphini</span> Star in the constellation Delphinus

1 Delphini is the Flamsteed designation for a close binary star in the equatorial constellation Delphinus. With a combined apparent magnitude of 6.08, it is barely visible to the naked eye, even under ideal conditions. Parallax measurements put the components at a distance 703 and 780 light years respectively. However, its approaching the Solar System with a radial velocity of 15 km/s.

16 Delphini is a star in the equatorial constellation Delphinus. It has an apparent magnitude of 5.54, making it faintly visible to the naked eye. The star is relatively close at a distance of 198 light years but is receding with a poorly constrained radial velocity of 2 km/s.

<span class="mw-page-title-main">Omega Octantis</span> Star in the constellation of Octans

Omega Octantis,, is a solitary, bluish-white hued star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.87, allowing it to be faintly seen with the naked eye. Based on the object's parallax measurements, it is estimated to be 328 light years distant. However, it is drifting closer with a heliocentric radial velocity −7.6 km/s.

<span class="mw-page-title-main">23 Leonis Minoris</span> Star in the constellation of Leo Minor

23 Leonis Minoris is a solitary, bluish-white hued star located in the northern constellation Leo Minor. It is positioned 7° south and 11" west from β Leonis Minoris. It is rarely called 7 H. Leonis Minoris, which is its Hevelius designation.

References

  1. Referred to as ApJ on its own website
  2. "American Astronomical Society Journals Going Electronic Only". IOP Publishing. 2014-06-02. Retrieved 2017-01-12.
  3. "American Astronomical Society Selects Institute of Physics Publishing As New Publishing Partner". PR Newswire Europe Ltd. 2007-04-25. Retrieved 2007-07-21.
  4. Howard, Jennifer (2007-05-18). "U. of Chicago Press Loses 3 Journals After Publishing Agreement Is Changed". Chronicle of Higher Education. Archived from the original on 2021-04-26. Retrieved 2009-02-12.
  5. Abt, Helmut (2009). "Reviewing and Revision Times for The Astrophysical Journal". Publications of the Astronomical Society of the Pacific. 121 (885): 1291–1293. Bibcode:2009PASP..121.1291A. doi: 10.1086/648536 . ISSN   0004-6280.
  6. Pattasch, S. R.; Praderie, F. (1988). "Comparison of astronomical journals" (PDF). The ESO Messenger. 53: 16. Bibcode:1988Msngr..53...16P. ISSN   0722-6691.
  7. "AAS Journals Will Switch to Open Access". American Astronomical Society (Press release). September 1, 2021.
  8. "AAS Journals Transition to Open Access". The American Astronomica Society. Retrieved 5 April 2023.
  9. The Astrophysical Journal. 1(1).
  10. 1 2 Hale, George Ellery (1895). "The Astrophysical Journal". The Astrophysical Journal. 1 (1): 80–84. Bibcode:1895ApJ.....1...80H. doi: 10.1086/140011 . ISSN   0004-637X.
  11. Abt, H A (1995). "Some Statistical Highlights of the Astrophysical Journal". The Astrophysical Journal. 455: 407. Bibcode:1995ApJ...455..407A. doi: 10.1086/176587 . ISSN   0004-637X.
  12. 1 2 3 Osterbrock, Donald E. (1995-01-01). "Founded in 1895 by George E. Hale and James E. Keeler: The Astrophysical Journal Centennial". The Astrophysical Journal. 438: 4–6. Bibcode:1995ApJ...438....1O. doi: 10.1086/175049 . ISSN   0004-637X.
  13. Helmut A. Abt (1 December 1995). "Obituary – Chandrasekhar, Subrahmanyan". The Astrophysical Journal. 454: 551. Bibcode:1995ApJ...454..551A. doi: 10.1086/176507 . ISSN   0004-637X.