A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY
(ProQuest: ... denotes formulae and/or non-USASCII text omitted)We report on the discovery of a new Milky Way (MW) companion stellar system located at ( alpha J2000, delta J2000) = (22 super(h)10 super(m)43 super(s).15, 14[degrees]56'58".8). The discovery was made using the eighth data rel...
Gespeichert in:
| Veröffentlicht in: | The Astrophysical journal 2013-04, Vol.767 (2), p.1-6 |
|---|---|
| Hauptverfasser: | , , , , , , , , , |
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | 6 |
|---|---|
| container_issue | 2 |
| container_start_page | 1 |
| container_title | The Astrophysical journal |
| container_volume | 767 |
| creator | Balbinot, E Santiago, B X da Costa, L Maia, M A G Majewski, S R NIDEVER, D Rocha-Pinto, H J Thomas, D Wechsler, R H YANNY, B |
| description | (ProQuest: ... denotes formulae and/or non-USASCII text omitted)We report on the discovery of a new Milky Way (MW) companion stellar system located at ( alpha J2000, delta J2000) = (22 super(h)10 super(m)43 super(s).15, 14[degrees]56'58".8). The discovery was made using the eighth data release of SDSS after applying an automated method to search for overdensities in the Baryon Oscillation Spectroscopic Survey footprint. Follow-up observations were performed using Canada-France-Hawaii-Telescope/MegaCam, which reveal that this system is comprised of an old stellar population, located at a distance of ... kpc, with a half-light radius of ... pc and a concentration parameter of c = log sub(10)(r sub(t)/r sub(c)) = 1.55. A systematic isochrone fit to its color-magnitude diagram resulted in log (age yr super(-1)) = ... and [Fe/H] = ... These quantities are typical of globular clusters in the MW halo. The newly found object is of low stellar mass, whose observed excess relative to the background is caused by 95 + or - 6 stars. The direct integration of its background decontaminated luminosity function leads to an absolute magnitude of M sub(v) = -1.21 + or - 0.66. The resulting surface brightness is mu sub(v) = 25.90 mag arcsec super(-2). Its position in the M sub(v) versus r sub(h) diagram lies close to AM4 and Koposov 1, which are identified as star clusters. The object is most likely a very faint star cluster-one of the faintest and lowest mass systems yet identified. |
| doi_str_mv | 10.1088/0004-637X/767/2/101 |
| format | Article |
| fullrecord | <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_1437409</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1753538050</sourcerecordid><originalsourceid>FETCH-LOGICAL-c387t-ce2cb103a50ca515962a4bf50139dd25b6d7551b74342b36ee3d126e146638f83</originalsourceid><addsrcrecordid>eNqN0EFPgzAUwPHGaOKcfgIvjScvSNtHW7iYEIIbGW7JYJk7NVBKxGxDKTv47YXMePb08l5-eYc_QveUPFHi-y4hxHMEyDdXCukylxJ6gSaUg-94wOUlmvyJa3Rj7ce4siCYoOcQL-Mtfk3SxQ5vwx2eh-kKZ3m4xlG6yfJ4jZMlzucxzlabYayXeBamYZQnEc4Wu1t0VRd7a-5-5xRtXuI8mjvpapZEYepo8GXvaMN0SQkUnOiCUx4IVnhlzQmFoKoYL0UlOael9MBjJQhjoKJMGOoJAX7twxQ9nP-2tm-U1U1v9Ltuj0eje0U9kB4JBvR4Rp9d-3UytleHxmqz3xdH056sopLDkIRw8g_KGBU-cDZQOFPdtdZ2plafXXMoum9FiRrrqzGmGtuqob5iw5HCD1scbvk</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1722168352</pqid></control><display><type>article</type><title>A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY</title><source>IOP Publishing Free Content</source><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Alma/SFX Local Collection</source><creator>Balbinot, E ; Santiago, B X ; da Costa, L ; Maia, M A G ; Majewski, S R ; NIDEVER, D ; Rocha-Pinto, H J ; Thomas, D ; Wechsler, R H ; YANNY, B</creator><creatorcontrib>Balbinot, E ; Santiago, B X ; da Costa, L ; Maia, M A G ; Majewski, S R ; NIDEVER, D ; Rocha-Pinto, H J ; Thomas, D ; Wechsler, R H ; YANNY, B ; Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><description>(ProQuest: ... denotes formulae and/or non-USASCII text omitted)We report on the discovery of a new Milky Way (MW) companion stellar system located at ( alpha J2000, delta J2000) = (22 super(h)10 super(m)43 super(s).15, 14[degrees]56'58".8). The discovery was made using the eighth data release of SDSS after applying an automated method to search for overdensities in the Baryon Oscillation Spectroscopic Survey footprint. Follow-up observations were performed using Canada-France-Hawaii-Telescope/MegaCam, which reveal that this system is comprised of an old stellar population, located at a distance of ... kpc, with a half-light radius of ... pc and a concentration parameter of c = log sub(10)(r sub(t)/r sub(c)) = 1.55. A systematic isochrone fit to its color-magnitude diagram resulted in log (age yr super(-1)) = ... and [Fe/H] = ... These quantities are typical of globular clusters in the MW halo. The newly found object is of low stellar mass, whose observed excess relative to the background is caused by 95 + or - 6 stars. The direct integration of its background decontaminated luminosity function leads to an absolute magnitude of M sub(v) = -1.21 + or - 0.66. The resulting surface brightness is mu sub(v) = 25.90 mag arcsec super(-2). Its position in the M sub(v) versus r sub(h) diagram lies close to AM4 and Koposov 1, which are identified as star clusters. The object is most likely a very faint star cluster-one of the faintest and lowest mass systems yet identified.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/767/2/101</identifier><language>eng</language><publisher>United States: Institute of Physics (IOP)</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; Automation ; Decontamination ; Galactic halos ; Luminosity ; Milky Way Galaxy ; Searching ; Star clusters ; Stars ; Texts</subject><ispartof>The Astrophysical journal, 2013-04, Vol.767 (2), p.1-6</ispartof><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c387t-ce2cb103a50ca515962a4bf50139dd25b6d7551b74342b36ee3d126e146638f83</citedby><cites>FETCH-LOGICAL-c387t-ce2cb103a50ca515962a4bf50139dd25b6d7551b74342b36ee3d126e146638f83</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27901,27902</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1437409$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Balbinot, E</creatorcontrib><creatorcontrib>Santiago, B X</creatorcontrib><creatorcontrib>da Costa, L</creatorcontrib><creatorcontrib>Maia, M A G</creatorcontrib><creatorcontrib>Majewski, S R</creatorcontrib><creatorcontrib>NIDEVER, D</creatorcontrib><creatorcontrib>Rocha-Pinto, H J</creatorcontrib><creatorcontrib>Thomas, D</creatorcontrib><creatorcontrib>Wechsler, R H</creatorcontrib><creatorcontrib>YANNY, B</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><title>A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY</title><title>The Astrophysical journal</title><description>(ProQuest: ... denotes formulae and/or non-USASCII text omitted)We report on the discovery of a new Milky Way (MW) companion stellar system located at ( alpha J2000, delta J2000) = (22 super(h)10 super(m)43 super(s).15, 14[degrees]56'58".8). The discovery was made using the eighth data release of SDSS after applying an automated method to search for overdensities in the Baryon Oscillation Spectroscopic Survey footprint. Follow-up observations were performed using Canada-France-Hawaii-Telescope/MegaCam, which reveal that this system is comprised of an old stellar population, located at a distance of ... kpc, with a half-light radius of ... pc and a concentration parameter of c = log sub(10)(r sub(t)/r sub(c)) = 1.55. A systematic isochrone fit to its color-magnitude diagram resulted in log (age yr super(-1)) = ... and [Fe/H] = ... These quantities are typical of globular clusters in the MW halo. The newly found object is of low stellar mass, whose observed excess relative to the background is caused by 95 + or - 6 stars. The direct integration of its background decontaminated luminosity function leads to an absolute magnitude of M sub(v) = -1.21 + or - 0.66. The resulting surface brightness is mu sub(v) = 25.90 mag arcsec super(-2). Its position in the M sub(v) versus r sub(h) diagram lies close to AM4 and Koposov 1, which are identified as star clusters. The object is most likely a very faint star cluster-one of the faintest and lowest mass systems yet identified.</description><subject>ASTRONOMY AND ASTROPHYSICS</subject><subject>Automation</subject><subject>Decontamination</subject><subject>Galactic halos</subject><subject>Luminosity</subject><subject>Milky Way Galaxy</subject><subject>Searching</subject><subject>Star clusters</subject><subject>Stars</subject><subject>Texts</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqN0EFPgzAUwPHGaOKcfgIvjScvSNtHW7iYEIIbGW7JYJk7NVBKxGxDKTv47YXMePb08l5-eYc_QveUPFHi-y4hxHMEyDdXCukylxJ6gSaUg-94wOUlmvyJa3Rj7ce4siCYoOcQL-Mtfk3SxQ5vwx2eh-kKZ3m4xlG6yfJ4jZMlzucxzlabYayXeBamYZQnEc4Wu1t0VRd7a-5-5xRtXuI8mjvpapZEYepo8GXvaMN0SQkUnOiCUx4IVnhlzQmFoKoYL0UlOael9MBjJQhjoKJMGOoJAX7twxQ9nP-2tm-U1U1v9Ltuj0eje0U9kB4JBvR4Rp9d-3UytleHxmqz3xdH056sopLDkIRw8g_KGBU-cDZQOFPdtdZ2plafXXMoum9FiRrrqzGmGtuqob5iw5HCD1scbvk</recordid><startdate>20130401</startdate><enddate>20130401</enddate><creator>Balbinot, E</creator><creator>Santiago, B X</creator><creator>da Costa, L</creator><creator>Maia, M A G</creator><creator>Majewski, S R</creator><creator>NIDEVER, D</creator><creator>Rocha-Pinto, H J</creator><creator>Thomas, D</creator><creator>Wechsler, R H</creator><creator>YANNY, B</creator><general>Institute of Physics (IOP)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OIOZB</scope><scope>OTOTI</scope></search><sort><creationdate>20130401</creationdate><title>A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY</title><author>Balbinot, E ; Santiago, B X ; da Costa, L ; Maia, M A G ; Majewski, S R ; NIDEVER, D ; Rocha-Pinto, H J ; Thomas, D ; Wechsler, R H ; YANNY, B</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c387t-ce2cb103a50ca515962a4bf50139dd25b6d7551b74342b36ee3d126e146638f83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>Automation</topic><topic>Decontamination</topic><topic>Galactic halos</topic><topic>Luminosity</topic><topic>Milky Way Galaxy</topic><topic>Searching</topic><topic>Star clusters</topic><topic>Stars</topic><topic>Texts</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Balbinot, E</creatorcontrib><creatorcontrib>Santiago, B X</creatorcontrib><creatorcontrib>da Costa, L</creatorcontrib><creatorcontrib>Maia, M A G</creatorcontrib><creatorcontrib>Majewski, S R</creatorcontrib><creatorcontrib>NIDEVER, D</creatorcontrib><creatorcontrib>Rocha-Pinto, H J</creatorcontrib><creatorcontrib>Thomas, D</creatorcontrib><creatorcontrib>Wechsler, R H</creatorcontrib><creatorcontrib>YANNY, B</creatorcontrib><creatorcontrib>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Balbinot, E</au><au>Santiago, B X</au><au>da Costa, L</au><au>Maia, M A G</au><au>Majewski, S R</au><au>NIDEVER, D</au><au>Rocha-Pinto, H J</au><au>Thomas, D</au><au>Wechsler, R H</au><au>YANNY, B</au><aucorp>Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY</atitle><jtitle>The Astrophysical journal</jtitle><date>2013-04-01</date><risdate>2013</risdate><volume>767</volume><issue>2</issue><spage>1</spage><epage>6</epage><pages>1-6</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>(ProQuest: ... denotes formulae and/or non-USASCII text omitted)We report on the discovery of a new Milky Way (MW) companion stellar system located at ( alpha J2000, delta J2000) = (22 super(h)10 super(m)43 super(s).15, 14[degrees]56'58".8). The discovery was made using the eighth data release of SDSS after applying an automated method to search for overdensities in the Baryon Oscillation Spectroscopic Survey footprint. Follow-up observations were performed using Canada-France-Hawaii-Telescope/MegaCam, which reveal that this system is comprised of an old stellar population, located at a distance of ... kpc, with a half-light radius of ... pc and a concentration parameter of c = log sub(10)(r sub(t)/r sub(c)) = 1.55. A systematic isochrone fit to its color-magnitude diagram resulted in log (age yr super(-1)) = ... and [Fe/H] = ... These quantities are typical of globular clusters in the MW halo. The newly found object is of low stellar mass, whose observed excess relative to the background is caused by 95 + or - 6 stars. The direct integration of its background decontaminated luminosity function leads to an absolute magnitude of M sub(v) = -1.21 + or - 0.66. The resulting surface brightness is mu sub(v) = 25.90 mag arcsec super(-2). Its position in the M sub(v) versus r sub(h) diagram lies close to AM4 and Koposov 1, which are identified as star clusters. The object is most likely a very faint star cluster-one of the faintest and lowest mass systems yet identified.</abstract><cop>United States</cop><pub>Institute of Physics (IOP)</pub><doi>10.1088/0004-637X/767/2/101</doi><tpages>6</tpages><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0004-637X |
| ispartof | The Astrophysical journal, 2013-04, Vol.767 (2), p.1-6 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1437409 |
| source | IOP Publishing Free Content; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
| subjects | ASTRONOMY AND ASTROPHYSICS Automation Decontamination Galactic halos Luminosity Milky Way Galaxy Searching Star clusters Stars Texts |
| title | A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-15T20%3A35%3A49IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=A%20NEW%20MILKY%20WAY%20HALO%20STAR%20CLUSTER%20IN%20THE%20SOUTHERN%20GALACTIC%20SKY&rft.jtitle=The%20Astrophysical%20journal&rft.au=Balbinot,%20E&rft.aucorp=Fermi%20National%20Accelerator%20Lab.%20(FNAL),%20Batavia,%20IL%20(United%20States)&rft.date=2013-04-01&rft.volume=767&rft.issue=2&rft.spage=1&rft.epage=6&rft.pages=1-6&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.1088/0004-637X/767/2/101&rft_dat=%3Cproquest_osti_%3E1753538050%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=1722168352&rft_id=info:pmid/&rfr_iscdi=true |