Our next stop probably needs no introduction: Sweep 11[degrees] northwest of Alpha Persei to find the famous Double Cluster, NGC 869 and NGC 884 (Stop 2), one of the finest binocular sights in the entire sky. The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative

2) corresponds to a stellar mass of 4.68 M ⊙. Sigma Persei Mirfak. Using this method, we find that the MF of Alpha Persei is well described by a two-stage distribution over the 0.1–0.62 M ⊙ and 0.62–4.68 M ⊙ mass range with α low = 0.50 ± 0.09 and α high = 2.32 ± 0.14. The Omicron Persei and Sigma Scorpii dust characteristics exemplify a continuum of characteristics observed along various lines of sight, depending on the local dust environemnts. Struve 163 Cassiopea. Al Kirkab Gamma Geminorum. Sigma Persei‎ (1 F) Stock 2‎ (2 F) T Trumpler 2‎ (2 F) Media in category "Perseus (constellation)" The following 83 files are in this category, out of 83 total. The two components of Eta Persei itself are designated Eta Persei A (officially named Miram / ˈ m aɪər æ m /, a recent name for the system) and B. Files are available under licenses specified on their description page. The system exhibits periodic RV variations of 579.8 +/- 2.4 days. Notice, Smithsonian Terms of The turnoff point in the CMD of Alpha Persei (Fig.

It is of interest to consider Omicron Persei and Sigma Scorpii dust in the context of the average extinction law of Cardelli et al (1989), here referred to as 'CCM', which depends on the R(v) parameter; this is defined as the ratio of total to selective extinction. From Wikimedia Commons, the free media repository, Sigma Persei (it); Sigma Persei (fr); Sigma Persei (sv); sigma Persei (pl); Sigma Persei (nb); Sigma Persei (nl); Sigma Persei (ru); Sigma Persei (en); Sigma Persei (de); Sigma Persei (pt); Sigma Persei (ga); Sigma Persei (es); 天船增四 (zh); Sigma Persei (da) stella nella costellazione di Perseo (it); étoile (fr); stjärna i stjärnbilden Perseus (sv); gwiazda w gwiazdozbiorze Perseusza (pl); Звезда в созвездии Персея (ru); Stern im Sternbild Perseus (de); estrela (pt); star in the constellation Perseus (en); bintang yang terletak di rasi bintang Perseus (id); réalta (ga) 35 Persei (da); 35 Persei (de); 35 Persei (sv); 35 Persei (en); 35 Persei (fr); 35 Persei (nb); 35 Persei (nl), https://commons.wikimedia.org/w/index.php?title=Category:Sigma_Persei&oldid=315084591, Creative Commons Attribution-ShareAlike License. Alpha Librae (Zubenelgenubi) Beta Monocerotis. Beta Scorpii. 19 Ophiuchi. Astrophysical Observatory. Eta Persei (η Persei, abbreviated Eta Per, η Per), is a binary star and the 'A' component of a triple star system (the 'B' component is the star HD 237009) in the constellation of Perseus.It is approximately 1331 light-years away from Earth.. All structured data from the file and property namespaces is available under the. 61 Ophiuchi. The system exhibits periodic RV variations of 579.8 +/- 2.4 days.
The monster’s bulbous head is formed by bright Mirfak and a ring of 6th magnitude stars; σ (sigma) Persei marks the hump of the beast, and δ (delta) marks the tip of the tail. The purpose of the survey is to search for low-amplitude and Gamma Leporis. We report the detection of an exoplanet candidate in orbit around sigma Persei from a radial velocity (RV) survey. 54 Leonis. Mirfak, Alpha Persei (α Per) is a yellow supergiant star located in the constellation Perseus. Use, Smithsonian

Jump to navigation Jump to search. Rigel - Beta Orionis. Eta Persei. The first IUE low dispersion spectra for Omicron Persei and Sigma Scorpii have been obtained and extinction curves from 1150 to 3250 A are presented. Juba (Algieba) Gamma Leonis. These deviations are more typical of dark clouds or diffuse lines of sight, rather than of bright nebula lines of sight. Eta Orionis.

Southeast of Alpha, Sigma ([sigma]) Persei is a nice binocular multiple, dominated by a distinctly yellow K-type giant. Omicron Persei lies behind the edge of a dark cloud, and its dust shows a broad bump shifted to shorter wavelengths, similar to other dark cloud lines of sight, but shows no deviation from the CCM average curve in the far UV. With an apparent magnitude of 1.806, it is the brightest… Read More »Mirfak, Acamar Achernar Acrux Adhara Albireo Alcor Alcyone Aldebaran Alderamin Algenib Algol Alhena Alioth Alkaid Almach Alnair Alnilam Alnitak Alpha Centauri Alphard Alphecca Alpheratz Altair Aludra Ankaa Anser Antares Arcturus Ascella Asterope Atlas Atria Avior Baten Kaitos Bellatrix Betelgeuse Bharani Canopus Capella Caph Castor Celaeno Deneb Denebola Diphda Dubhe Electra Elnath Eltanin Enif Fomalhaut Gacrux Gamma Cassiopeiae Ginan Hadar Hamal Imai Izar Kaus Australis Kaus Borealis Kaus Media Maia Marfik Markab Megrez Meissa Menkalinan Menkar Menkent Merak Merope Mesarthim Miaplacidus Mimosa Mintaka Mira Mirach Mirfak Mirzam Mizar Mu Cephei Naos Nunki Peacock Phecda Pleione Polaris Pollux Procyon Proxima Centauri Rasalhague Regulus Rho Ophiuchi Rigel Rigil Kentaurus Ruchbah Sabik Sadr Saiph Sargas Scheat Schedar Segin Seginus Shaula Sheratan Sirius Spica Stephenson 2-18 Suhail Taygeta Thuban Toliman Unukalhai UY Scuti Vega VV Cephei VX Sagittarii Wezen WOH G64 Zeta Reticuli Zubenelgenubi Zubeneschamali. Sigma Persei (35 Persei) é uma estrela na direção da constelação de Perseus.Possui uma ascensão reta de 03h 30m 34.48s e uma declinação de +47° 59′ 42.6″. Pertence à classe espectral K3III.. Ver também Castor Gamma Geminorum. Considerando sua distância de 353 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.93. This page was last edited on 17 August 2018, at 14:14. by admin; Posted on 2019-10-20 2020-08-31; Lucidae; Mirfak, Alpha Persei (α Per) is a yellow supergiant star located in the constellation Perseus. The system exhibits periodic RV variations of 579.8 +/- 2.4 days.

From Wikimedia Commons, the free media repository. Agreement NNX16AC86A, Is ADS down? The first IUE low dispersion spectra for Omicron Persei and Sigma Scorpii have been obtained and extinction curves from 1150 to 3250 A are presented. Sua magnitude aparente é igual a 4.36.
Sigma Orionis. Sigma Cassiopeiae. (or is it just me...), Smithsonian Privacy Sigma Scorpii lies within the H II region near a dark cloud, and its dust shows a marked deviation from the CCM law in the far UV.

This category contains only the following file. We report the detection of an exoplanet candidate in orbit around sigma Persei from a radial velocity (RV) survey. 2011-08-02 00-32-00-constellations.jpg 3,201 × 5,745; 15.94 MB. H 3752 Lepus. Sigma Persei has an 6 1/2 Jupiter Mass ExoPlanet at 1.8 AU Planetary companion in K giant Sigma Persei Authors: Lee et al Abstract: We report the detection of an exoplanet candidate in orbit around sigma Persei from a radial velocity (RV) survey. Category:Sigma Persei. Albireo beta Cygni. With an apparent magnitude of 1.806, it is the brightest star in Perseus, outshining the more famous Algol, and the …


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