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Globular cluster in the constellation Horologium
Arp-Madore 1 (also known as AM 1) is a globular cluster visible in the constellation Horologium, located 123.3 kiloparsecs (402,000 light-years) away from
Arp-Madore_1
Open cluster in Puppis
Arp-Madore 2 (also known as AM 2) is an open cluster of stars in the constellation of Puppis. It is almost 30,000 light-years away and about 5 billion
Arp-Madore_2
Topics referred to by the same term
a 1918 U.S. Navy minesweeper AM-1, a designation of the 1946 AM Mauler aircraft Arp-Madore 1, a star-cluster АМ-1, "Атом Мирный", the first civilian
AM1
Ring galaxy
Arp-Madore 417-391 is a ring galaxy located 671 million light-years from Earth in the constellation of Eridanus. It is classified as a ring galaxy. The
Arp-Madore_417-391
List from the Alphabet Direction (αβ)
open and globular star clusters (Halton Arp / Barry F. Madore) (for example: Arp-Madore 1 in Horologium, Arp-Madore 2 in Puppis) An — Anderson (double stars)
List of astronomical catalogues
List_of_astronomical_catalogues
Constellation in the southern celestial hemisphere
lies 4.7 degrees north-northeast of Mu Horologii. The globular cluster Arp-Madore 1 is the most remote known globular cluster in the Milky Way at a distance
Horologium_(constellation)
Star in the constellation Horologium
Exoplanets HD 27631 b ι Horologii b Star clusters NGC 1252 1261 Other Arp-Madore 1 Galaxies NGC 888 1249 1311 1356 1433 1448 1483 1493 1510 1512 1527 Other
Zeta_Horologii
Binary star system in the constellation Horologium
an equatorial bulge that is 15% larger than the polar radius. The star has 1.4 times the mass of the Sun. The secondary has an apparent magnitude of 7
Delta_Horologii
Elliptical galaxy in the constellation Hydra
of galaxies also appears in the Catalog of Collisional Ring Galaxies by Madore, Nelson and Petrillo. James Webb Space Telescope image of NGC 2937. Hubble
NGC_2937
Binary star system in the constellation Horologium
Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966
Eta_Horologii
Star in the constellation Horologium
Michigan catalogue of two-dimensional spectral types for the HD stars, vol. 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode:1978mcts
Gamma_Horologii
Galactic Center are right ascension 17h 45m 40.04s, declination −29° 00′ 28.1″. A high proportion of globular clusters are located in the Ophiuchus and
List_of_globular_clusters
Interacting galaxies in the constellation Cetus
"Neutral hydrogen observations of ARP 144". The Astrophysical Journal. 326: 146. doi:10.1086/166075. ISSN 0004-637X. Madore, Barry F.; Nelson, Erica; Petrillo
Arp_146
Interacting ring galaxy in Microscopium
and Associations (AM Catalogue), compiled by astronomers Halton Arp and Barry F. Madore in 1987. It consists of two principal galactic components or nuclei:
AM_2026-424
Star in the constellation Horologium
years old with a projected rotational velocity of 79.2 km/s. The star has 1.5 times the mass of the Sun and is radiating 13 times the solar luminosity
Mu_Horologii
Group of galaxies in the constellation Leo
Kennicutt Jr., J. R. Mould, S. Sakai, W. L. Freedman, P. B. Stetson, B. F. Madore, B. K. Gibson, J. A. Graham, S. M. Hughes, G. D. Illingworth, D. D. Kelson
Leo_Triplet
Star in the constellation Horologium
Plate". The Astrophysical Journal. 800 (1): 5. arXiv:1412.5179. Bibcode:2015ApJ...800....5M. doi:10.1088/0004-637X/800/1/5. S2CID 119211833. 5. Rhee, Joseph
Nu_Horologii
Galaxy in the constellation Cetus
surface brightness galaxies are Arp 1 (NGC 2857), Arp 2 (UGC 10310), Arp 3, Arp 5 (NGC 3664), and Arp 6 (NGC 2537). Arp 4 has a possible active galactic
Arp_4
Radio galaxy in the constellation Centaurus
Strasbourg. Retrieved 29 November 2009. Armando, Gil de Paz; Boissier; Madore; Seibert; Boselli; et al. (2007). "The GALEX Ultraviolet Atlas of Nearby
Centaurus_A
American astronomer (1927-2013)
Barry F. Madore (1987) Cosmology Non-standard cosmology Intrinsic redshifts Redshift quantization Le Sage's theory of gravitation Halton Arp, Seeing Red:
Halton_Arp
Galaxy in the constellation Horologium
credit: European Space Agency)". nasa.gov. Retrieved 2021-01-10. Arp, H.C.; Madore, B.F; Roberton, W. "A Catalogue of Southern Peculiar Galaxies and
NGC_1356
Ring galaxy in the constellation of Volans
another 300 million years, after which it will begin to disintegrate. Arp-Madore 417-391 ESO 69-6 PGC 6240 Hoag's Object "Nasa/Ipac Extragalactic Database"
AM_0644−741
Galaxy in the constellation Ursa Major
Strasbourg. Retrieved 2009-11-29. Gil de Paz, Armando; Boissier, Samuel; Madore, Barry F.; Seibert, Mark; et al. (December 2007). "The GALEX Ultraviolet
Pinwheel_Galaxy
Galaxy in the constellation Ursa Major
Strasbourg. Retrieved 14 December 2018. Armando, Gil de Paz; Boissier; Madore; Seibert; Boselli; et al. (2007). "The GALEX Ultraviolet Atlas of Nearby
Messier_82
Solitary red clump giant star in the constellation Eridanus
1692 1700 1721 1723 1725 1728 1741 Other Abell 402 BCG Abell 521 BCG Arp 187 Arp-Madore 417-391 Eridanus II ESO 0313−192 ESO 198-13 HE 0435−1223 IC 1953 IC
Iota_Eridani
Galaxies in the constellation Corvus
....D. ISBN 0-387-97552-7. Schweizer, François; Burns, Christopher R.; Madore, Barry F.; Mager, Violet A.; Phillips, M. M.; Freedman, Wendy L.; Boldt
Antennae_Galaxies
Variable star in the constellation Eridanus
rapidly with a projected rotational velocity of 108.1 km/s and a rotation period of less than around 1.9 days. This is creating an equatorial bulge that
Omicron1_Eridani
Star in the constellation Eridanus
G-type subgiant star with a stellar classification of G8 IV. It is about 1.6 times the mass of the Sun and has 4 times the Sun's radius. The star shines
Chi_Eridani
K-type giant star in the constellation Eridanus
binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209. Zhao, G.; et al. (2001). "High-Resolution
Rho1_Eridani
Star in the constellation Eridanus
1692 1700 1721 1723 1725 1728 1741 Other Abell 402 BCG Abell 521 BCG Arp 187 Arp-Madore 417-391 Eridanus II ESO 0313−192 ESO 198-13 HE 0435−1223 IC 1953 IC
Tau2_Eridani
Dwarf elliptical galaxy in the constellation Andromeda
astronomiques de Strasbourg. Retrieved 2009-11-29. Armando, Gil de Paz; Boissier; Madore; Seibert; Boselli; et al. (2007). "The GALEX Ultraviolet Atlas of Nearby
Messier_32
Minor constellation in the southern celestial hemisphere
times the Sun's mass located 223 ± 8 light-years distant. It passed within 1.14 and 3.45 light-years of the Sun some 3.9 million years ago, possibly disturbing
Microscopium
Star in the constellation Puppis
surface gravity are 5.8 R☉, 13,000 K and 3.4 cgs. Nu Puppis is located within 1° of the precession circle of the southern celestial pole. From around 13300
Nu_Puppis
Star in the constellation Eridanus
Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966
Rho3_Eridani
Astronomical objects
more galaxies colliding. The Cartwheel Galaxy, galaxy pair AM 2026-424, and Arp 147 are all examples of ring galaxies believed to be formed from this process
List_of_ring_galaxies
Binary star system in the constellation Eridanus
magnitude over the range 3.57−3.72 with a periodicity of 23.8 d. This star has 1.73 times the mass of the Sun and 103 times the radius of the Sun. It shines
Tau4_Eridani
A-type star in the constellation Eridanus
The Astrophysical Journal, 768 (1): 29, arXiv:1211.1415, Bibcode:2013ApJ...768...25G, doi:10.1088/0004-637X/768/1/25, S2CID 119295265, 25. Van Belle
Tau3_Eridani
Star in the constellation Eridanus
Astronomy University of Chile, 1, Publicaciones Universidad de Chile, Department de Astronomy: 1–17, Bibcode:1966PDAUC...1....1G. Zorec, J.; Royer, F. (2012)
Tau7_Eridani
Variable star in the constellation Eridanus
magnitude of −2.84. (Currently, the brightest star is Sirius at magnitude −1.46.) This is a B-type subgiant star with a stellar classification of B1.5 IV
Nu_Eridani
Star in the constellation Eridanus
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by: 2 ⋅ R ∗ = ( 155.8 ⋅ 0.346
Kappa_Eridani
Variable star in the constellation Eridanus
1692 1700 1721 1723 1725 1728 1741 Other Abell 402 BCG Abell 521 BCG Arp 187 Arp-Madore 417-391 Eridanus II ESO 0313−192 ESO 198-13 HE 0435−1223 IC 1953 IC
Mu_Eridani
Variable Star in the constellation Puppis
kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966
Omicron_Puppis
Variable star in the constellation Eridanus
B-type star that undergoes radial-velocity variation with a frequency of 1.1569 times per day. The star has about five times the mass of the Sun and
Tau8_Eridani
Star in the constellation Eridanus
sequence star and a subgiant. It has an estimated 140% of the Sun's mass and 1.73 times the radius of the Sun. The star is radiating 5.29 times the luminosity
Tau6_Eridani
F-type main sequence star in the constellation Eridanus
(May 2017). "Characterizing 51 Eri b from 1 to 5μm: a partly-cloudy exoplanet". The Astronomical Journal. 154 (1): 10. arXiv:1705.03887. Bibcode:2017AJ.
51_Eridani
Red giant star in the constellation Eridanus
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3 ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by: 2 ⋅ R ∗ = ( 150 ⋅ 4.8 ⋅
Pi_Eridani
Star in the constellation Eridanus
Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, arXiv:1208.2037, Bibcode:2012MNRAS.427..343M, doi:10.1111/j.1365-2966
Upsilon3_Eridani
Star in the constellation Eridanus
Heidelberg, 35, Veröffentlichungen des Astronomisches Rechen-Institut Heidelberg: 1, Bibcode:1999VeARI..35....1W. Eggen, Olin J. (August 1998), "The Sirius Supercluster
Xi_Eridani
Red clump star in the constellation Eridanus
K0III-IV. The measured angular diameter, after correction for limb darkening, is 1.74±0.02 mas. At an estimated distance of this star, this yields a physical
Upsilon1_Eridani
Binary star in the constellation Eridanus
component Tau9 Eridani A has an estimated 326% the mass of the Sun and 3.1 times the Sun's radius. It shines with 166 times the solar luminosity from
Tau9_Eridani
Star in the constellation Eridanus
Astrophysical formulae, Astronomy and astrophysics library, vol. 1 (3rd ed.), Birkhäuser, ISBN 3-540-29692-1. The radius (R*) is given by: 2 ⋅ R ∗ = ( 72 ⋅ 0.87 ⋅
Omega_Eridani
Star in the constellation Eridanus
1692 1700 1721 1723 1725 1728 1741 Other Abell 402 BCG Abell 521 BCG Arp 187 Arp-Madore 417-391 Eridanus II ESO 0313−192 ESO 198-13 HE 0435−1223 IC 1953 IC
Upsilon4_Eridani
Star in the constellation of Eridanus
names for stars. The WGSN approved the name Theemin for this star on February 1, 2017, and it is now included in the List of IAU-approved Star Names. In the
Upsilon2_Eridani
Binary star system in the constellation Eridanus
The Astrophysical Journal, 792 (1): 19, arXiv:1407.4579, Bibcode:2014ApJ...792...65P, doi:10.1088/0004-637X/792/1/65, S2CID 119282523, 65. Gáspár, András;
Zeta_Eridani
Variable star in the constellation Eridanus
class of variable is uncertain. The Gaia EDR3 data identified a comoving 0.1 M☉ companion star of Gamma Eridani, at a projected separation of 1000 AU.
Gamma_Eridani
K-type giant star in the constellation Eridanus
2 s−1", Astronomische Nachrichten, 321 (1): 1–52, arXiv:astro-ph/0003039, Bibcode:2000AN....321....1S, doi:10.1002/(SICI)1521-3994(200003)321:1<1::AID-ASNA1>3
Rho2_Eridani
Variable star in the constellation Eridanus
likely rotation period is deemed to be twice the period of variation, or 1.4 days. The star also possesses a rotating circumstellar disc, seen edge on
Lambda_Eridani
Barred spiral galaxy in the Local Group
31". Retrieved 30 September 2018. Gil de Paz, Armando; Boissier, Samuel; Madore, Barry F.; et al. (2007). "The GALEX Ultraviolet Atlas of Nearby Galaxies"
Andromeda_Galaxy
Star in the constellation Eridanus
kpc from the Sun", Monthly Notices of the Royal Astronomical Society, 410 (1): 190–200, arXiv:1007.4883, Bibcode:2011MNRAS.410..190T, doi:10.1111/j.1365-2966
Psi_Eridani
Galaxy in the constellation Canes Venatici
Parise, Ronald A.; Smith, Eric P.; Freedman, Wendy L.; Kuchinski, Leslie E.; Madore, Barry; Angione, Ronald; Palma, Christopher; Talbert, Freddie; Stecher,
NGC_4156
White dwarf in the constellation Puppis
Members of the 25 parsec White Dwarf Sample". The Astronomical Journal. 154 (1): 32. arXiv:1706.00709. Bibcode:2017AJ....154...32S. doi:10.3847/1538-3881/aa76e0
WD_0816−310
Binary star in the constellation Eridanus
WISEA J044634.16-262756.1 (also known as J0446) is a binary star system with one component having a long-lived primordial disk, also called a Peter Pan
WISEA_J044634.16-262756.1
Star in the constellation Eridanus
early-type binaries", Monthly Notices of the Royal Astronomical Society, 392 (1): 448–454, Bibcode:2009MNRAS.392..448H, doi:10.1111/j.1365-2966.2008.14073
Tau5_Eridani
Blue-hued star in the constellation Eridanus
Catalogue", The Astrophysical Journal Supplement, 192 (1): 2, arXiv:1007.0425, Bibcode:2011ApJS..192....2S, doi:10.1088/0067-0049/192/1/2, S2CID 119226823.
Phi_Eridani
Governor of New York from 2007 to 2008
Archived from the original on December 24, 2010. Retrieved November 14, 2007. Madore, James T. (November 9, 2007). "Spitzer defends license plan over Democrat
Eliot_Spitzer
Galaxy with a high luminosity
Bridge, C. R.; Chan, B.; Frayer, D.; Iwasawa, K.; Kewley, L. J.; Lord, S.; Madore, B. F.; Melbourne, J. E.; Murphy, E. J.; Rich, J. A.; Schulz, B.; et al
Luminous_infrared_galaxy
Constellation split into two non-contiguous parts
objects include Seyfert's Sextet, one of the densest galaxy clusters known; Arp 220, the prototypical ultraluminous infrared galaxy; and Hoag's Object, the
Serpens
The Astrophysical Journal. 698 (1): 1–27. arXiv:0903.2666. Bibcode:2009ApJ...698....1C. doi:10.1088/0004-637X/698/1/1. S2CID 9207187. Bonatto, C.; Bica
List_of_open_clusters
Portion of the giant branch before helium ignition
1051/0004-6361/201016066. S2CID 56067351. Lee, Myung Gyoon; Freedman, Wendy L.; Madore, Barry F. (1993). "The Tip of the Red Giant Branch as a Distance Indicator
Red-giant_branch
QSO 1213-0017 at z=1.31 (the quasar lies at z=2.69) In 1999, cluster RDCS J0849+4452 (RX J0849+4452, RXJ0848.9+4452) was found at z=1.261 In 1995 and 2001
List of galaxy groups and clusters
List_of_galaxy_groups_and_clusters
Galaxy merger in the constellation Boötes
1093/mnras/214.2.87. ISSN 0035-8711. Sanders, D. B.; Soifer, B. T.; Elias, J. H.; Madore, B. F.; Matthews, K.; Neugebauer, G.; Scoville, N. Z. (1988-02-01). "Ultraluminous
PKS_1345+125
American astronomer and astrophotographer
; Bardalez-Gagliuffi, Daniella C; Peñarrubia, Jorge; Chonis, Taylor S; Madore, Barry; Trujillo, Ignacio; Schirmer, Mischa; McDavid, David A (2010). "Stellar
R._Jay_GaBany
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