THE W40 REGION IN THE GOULD BELT: AN EMBEDDED CLUSTER AND H II REGION AT THE JUNCTION OF FILAMENTS

We present a multiwavelength study of the W40 star-forming region using infrared (IR) observations in the UKIRT JHK bands, Spitzer Infrared Array Camera bands, and Herschel PACS bands, 2.12 mu m H sub(2) narrowband imaging, and radio continuum observations from GMRT (610 and 1280 MHz), in a field of...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2013-12, Vol.779 (2), p.1-17
Hauptverfasser: Mallick, K K, Kumar, M S N, Ojha, D K, Bachiller, Rafael, Samal, M R, Pirogov, L
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 17
container_issue 2
container_start_page 1
container_title The Astrophysical journal
container_volume 779
creator Mallick, K K
Kumar, M S N
Ojha, D K
Bachiller, Rafael
Samal, M R
Pirogov, L
description We present a multiwavelength study of the W40 star-forming region using infrared (IR) observations in the UKIRT JHK bands, Spitzer Infrared Array Camera bands, and Herschel PACS bands, 2.12 mu m H sub(2) narrowband imaging, and radio continuum observations from GMRT (610 and 1280 MHz), in a field of view (FoV) of ~34' x 40'. Archival Spitzer observations in conjunction with near-IR observations are used to identify 1162 Class II/III and 40 Class I sources in the FoV. The nearest-neighbor stellar surface density analysis shows that the majority of these young stellar objects (YSOs) constitute the embedded cluster centered on the high-mass source IRS 1A South. Radio continuum analysis shows that this region has a blister morphology, with the radio peak coinciding with a protostellar source.
doi_str_mv 10.1088/0004-637X/779/2/113
format Article
fullrecord <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22348449</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1705085104</sourcerecordid><originalsourceid>FETCH-LOGICAL-c488t-89538df023f738239eaa8c9d83b00597d2c2437dcfa8e081925cc96ffbc908c13</originalsourceid><addsrcrecordid>eNqNkU1Lw0AQhhdRsH78Ai8LXvQQO_uR7q632GzbSExBU_S2pNsNRmpTs1Hw35tY9expmJfnHQYehM4IXBGQcggAPBgx8TQUQg3pkBC2hwYkZDLgLBT7aPBHHKIj71_6lSo1QMt8pvEjB3yvp8k8w0mG-2Q6X6QxvtFpfo2jDOu7Gx3HOsbjdPGQ6_sui_EMJ8lvLcq_a7eLbJz3-3yCJ0ka3eksfzhBB2Wx9u70Zx6jxUTn41mQzqfJOEoDy6VsA6m6d1clUFYKJilTriikVSvJlgChEitqKWdiZctCOpBE0dBaNSrLpVUgLWHH6Hx3t_ZtZbytWmefbb3ZONsaShmXnKuOutxRz8XabJvqtWg-TV1UZhalps-AcKbCkH_0Fy927Lap396db81r5a1br4uNq9-9IYJINRIjYP9AIQQZEuAdynaobWrvG1f-vUHA9DpNb8f0skyn01DT6WRfevyGSw</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1705085104</pqid></control><display><type>article</type><title>THE W40 REGION IN THE GOULD BELT: AN EMBEDDED CLUSTER AND H II REGION AT THE JUNCTION OF FILAMENTS</title><source>IOP Publishing Free Content</source><source>EZB-FREE-00999 freely available EZB journals</source><source>Alma/SFX Local Collection</source><creator>Mallick, K K ; Kumar, M S N ; Ojha, D K ; Bachiller, Rafael ; Samal, M R ; Pirogov, L</creator><creatorcontrib>Mallick, K K ; Kumar, M S N ; Ojha, D K ; Bachiller, Rafael ; Samal, M R ; Pirogov, L</creatorcontrib><description>We present a multiwavelength study of the W40 star-forming region using infrared (IR) observations in the UKIRT JHK bands, Spitzer Infrared Array Camera bands, and Herschel PACS bands, 2.12 mu m H sub(2) narrowband imaging, and radio continuum observations from GMRT (610 and 1280 MHz), in a field of view (FoV) of ~34' x 40'. Archival Spitzer observations in conjunction with near-IR observations are used to identify 1162 Class II/III and 40 Class I sources in the FoV. The nearest-neighbor stellar surface density analysis shows that the majority of these young stellar objects (YSOs) constitute the embedded cluster centered on the high-mass source IRS 1A South. Radio continuum analysis shows that this region has a blister morphology, with the radio peak coinciding with a protostellar source.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/779/2/113</identifier><language>eng</language><publisher>United States: American Astronomical Society</publisher><subject>Arrays ; Astrophysics ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Bands ; Clusters ; CONNECTORS ; Continuums ; DENSITY ; ELECTRIC CONTACTS ; ENERGY SPECTRA ; FILAMENTS ; FLUORESCENCE ; Infrared ; MASS ; PERTURBED ANGULAR CORRELATION ; PHOTOIONIZATION ; PROTOSTARS ; Radio ; Sciences of the Universe ; SEMICONDUCTOR JUNCTIONS ; STARS ; SUPERCONDUCTING JUNCTIONS ; SURFACES</subject><ispartof>The Astrophysical journal, 2013-12, Vol.779 (2), p.1-17</ispartof><rights>Distributed under a Creative Commons Attribution 4.0 International License</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c488t-89538df023f738239eaa8c9d83b00597d2c2437dcfa8e081925cc96ffbc908c13</citedby><cites>FETCH-LOGICAL-c488t-89538df023f738239eaa8c9d83b00597d2c2437dcfa8e081925cc96ffbc908c13</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,778,782,883,27907,27908</link.rule.ids><backlink>$$Uhttps://hal.science/hal-01439554$$DView record in HAL$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/22348449$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Mallick, K K</creatorcontrib><creatorcontrib>Kumar, M S N</creatorcontrib><creatorcontrib>Ojha, D K</creatorcontrib><creatorcontrib>Bachiller, Rafael</creatorcontrib><creatorcontrib>Samal, M R</creatorcontrib><creatorcontrib>Pirogov, L</creatorcontrib><title>THE W40 REGION IN THE GOULD BELT: AN EMBEDDED CLUSTER AND H II REGION AT THE JUNCTION OF FILAMENTS</title><title>The Astrophysical journal</title><description>We present a multiwavelength study of the W40 star-forming region using infrared (IR) observations in the UKIRT JHK bands, Spitzer Infrared Array Camera bands, and Herschel PACS bands, 2.12 mu m H sub(2) narrowband imaging, and radio continuum observations from GMRT (610 and 1280 MHz), in a field of view (FoV) of ~34' x 40'. Archival Spitzer observations in conjunction with near-IR observations are used to identify 1162 Class II/III and 40 Class I sources in the FoV. The nearest-neighbor stellar surface density analysis shows that the majority of these young stellar objects (YSOs) constitute the embedded cluster centered on the high-mass source IRS 1A South. Radio continuum analysis shows that this region has a blister morphology, with the radio peak coinciding with a protostellar source.</description><subject>Arrays</subject><subject>Astrophysics</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Bands</subject><subject>Clusters</subject><subject>CONNECTORS</subject><subject>Continuums</subject><subject>DENSITY</subject><subject>ELECTRIC CONTACTS</subject><subject>ENERGY SPECTRA</subject><subject>FILAMENTS</subject><subject>FLUORESCENCE</subject><subject>Infrared</subject><subject>MASS</subject><subject>PERTURBED ANGULAR CORRELATION</subject><subject>PHOTOIONIZATION</subject><subject>PROTOSTARS</subject><subject>Radio</subject><subject>Sciences of the Universe</subject><subject>SEMICONDUCTOR JUNCTIONS</subject><subject>STARS</subject><subject>SUPERCONDUCTING JUNCTIONS</subject><subject>SURFACES</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNqNkU1Lw0AQhhdRsH78Ai8LXvQQO_uR7q632GzbSExBU_S2pNsNRmpTs1Hw35tY9expmJfnHQYehM4IXBGQcggAPBgx8TQUQg3pkBC2hwYkZDLgLBT7aPBHHKIj71_6lSo1QMt8pvEjB3yvp8k8w0mG-2Q6X6QxvtFpfo2jDOu7Gx3HOsbjdPGQ6_sui_EMJ8lvLcq_a7eLbJz3-3yCJ0ka3eksfzhBB2Wx9u70Zx6jxUTn41mQzqfJOEoDy6VsA6m6d1clUFYKJilTriikVSvJlgChEitqKWdiZctCOpBE0dBaNSrLpVUgLWHH6Hx3t_ZtZbytWmefbb3ZONsaShmXnKuOutxRz8XabJvqtWg-TV1UZhalps-AcKbCkH_0Fy927Lap396db81r5a1br4uNq9-9IYJINRIjYP9AIQQZEuAdynaobWrvG1f-vUHA9DpNb8f0skyn01DT6WRfevyGSw</recordid><startdate>20131220</startdate><enddate>20131220</enddate><creator>Mallick, K K</creator><creator>Kumar, M S N</creator><creator>Ojha, D K</creator><creator>Bachiller, Rafael</creator><creator>Samal, M R</creator><creator>Pirogov, L</creator><general>American Astronomical Society</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>1XC</scope><scope>OTOTI</scope></search><sort><creationdate>20131220</creationdate><title>THE W40 REGION IN THE GOULD BELT: AN EMBEDDED CLUSTER AND H II REGION AT THE JUNCTION OF FILAMENTS</title><author>Mallick, K K ; Kumar, M S N ; Ojha, D K ; Bachiller, Rafael ; Samal, M R ; Pirogov, L</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c488t-89538df023f738239eaa8c9d83b00597d2c2437dcfa8e081925cc96ffbc908c13</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Arrays</topic><topic>Astrophysics</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Bands</topic><topic>Clusters</topic><topic>CONNECTORS</topic><topic>Continuums</topic><topic>DENSITY</topic><topic>ELECTRIC CONTACTS</topic><topic>ENERGY SPECTRA</topic><topic>FILAMENTS</topic><topic>FLUORESCENCE</topic><topic>Infrared</topic><topic>MASS</topic><topic>PERTURBED ANGULAR CORRELATION</topic><topic>PHOTOIONIZATION</topic><topic>PROTOSTARS</topic><topic>Radio</topic><topic>Sciences of the Universe</topic><topic>SEMICONDUCTOR JUNCTIONS</topic><topic>STARS</topic><topic>SUPERCONDUCTING JUNCTIONS</topic><topic>SURFACES</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mallick, K K</creatorcontrib><creatorcontrib>Kumar, M S N</creatorcontrib><creatorcontrib>Ojha, D K</creatorcontrib><creatorcontrib>Bachiller, Rafael</creatorcontrib><creatorcontrib>Samal, M R</creatorcontrib><creatorcontrib>Pirogov, L</creatorcontrib><collection>CrossRef</collection><collection>Meteorological &amp; Geoastrophysical Abstracts</collection><collection>Meteorological &amp; Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Hyper Article en Ligne (HAL)</collection><collection>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mallick, K K</au><au>Kumar, M S N</au><au>Ojha, D K</au><au>Bachiller, Rafael</au><au>Samal, M R</au><au>Pirogov, L</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE W40 REGION IN THE GOULD BELT: AN EMBEDDED CLUSTER AND H II REGION AT THE JUNCTION OF FILAMENTS</atitle><jtitle>The Astrophysical journal</jtitle><date>2013-12-20</date><risdate>2013</risdate><volume>779</volume><issue>2</issue><spage>1</spage><epage>17</epage><pages>1-17</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><abstract>We present a multiwavelength study of the W40 star-forming region using infrared (IR) observations in the UKIRT JHK bands, Spitzer Infrared Array Camera bands, and Herschel PACS bands, 2.12 mu m H sub(2) narrowband imaging, and radio continuum observations from GMRT (610 and 1280 MHz), in a field of view (FoV) of ~34' x 40'. Archival Spitzer observations in conjunction with near-IR observations are used to identify 1162 Class II/III and 40 Class I sources in the FoV. The nearest-neighbor stellar surface density analysis shows that the majority of these young stellar objects (YSOs) constitute the embedded cluster centered on the high-mass source IRS 1A South. Radio continuum analysis shows that this region has a blister morphology, with the radio peak coinciding with a protostellar source.</abstract><cop>United States</cop><pub>American Astronomical Society</pub><doi>10.1088/0004-637X/779/2/113</doi><tpages>17</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2013-12, Vol.779 (2), p.1-17
issn 0004-637X
1538-4357
language eng
recordid cdi_osti_scitechconnect_22348449
source IOP Publishing Free Content; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection
subjects Arrays
Astrophysics
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Bands
Clusters
CONNECTORS
Continuums
DENSITY
ELECTRIC CONTACTS
ENERGY SPECTRA
FILAMENTS
FLUORESCENCE
Infrared
MASS
PERTURBED ANGULAR CORRELATION
PHOTOIONIZATION
PROTOSTARS
Radio
Sciences of the Universe
SEMICONDUCTOR JUNCTIONS
STARS
SUPERCONDUCTING JUNCTIONS
SURFACES
title THE W40 REGION IN THE GOULD BELT: AN EMBEDDED CLUSTER AND H II REGION AT THE JUNCTION OF FILAMENTS
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-16T09%3A29%3A12IST&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=THE%20W40%20REGION%20IN%20THE%20GOULD%20BELT:%20AN%20EMBEDDED%20CLUSTER%20AND%20H%20II%20REGION%20AT%20THE%20JUNCTION%20OF%20FILAMENTS&rft.jtitle=The%20Astrophysical%20journal&rft.au=Mallick,%20K%20K&rft.date=2013-12-20&rft.volume=779&rft.issue=2&rft.spage=1&rft.epage=17&rft.pages=1-17&rft.issn=0004-637X&rft.eissn=1538-4357&rft_id=info:doi/10.1088/0004-637X/779/2/113&rft_dat=%3Cproquest_osti_%3E1705085104%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=1705085104&rft_id=info:pmid/&rfr_iscdi=true