THE KINEMATICS OF HH 34 FROM HST IMAGES WITH A NINE-YEAR TIME BASELINE

We study archival HST [SII] 6716+30 and H alpha images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The ~9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:The Astrophysical journal 2012-04, Vol.748 (2), p.1-10
Hauptverfasser: RAGA, A. C, NORIEGA-CRESPO, A, RODRIGUEZ-GONZALEZ, A, LORA, V, STAPELFELDT, K. R, CAREY, S. J
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page 10
container_issue 2
container_start_page 1
container_title The Astrophysical journal
container_volume 748
creator RAGA, A. C
NORIEGA-CRESPO, A
RODRIGUEZ-GONZALEZ, A
LORA, V
STAPELFELDT, K. R
CAREY, S. J
description We study archival HST [SII] 6716+30 and H alpha images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The ~9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the HH 34S bow shock (from the [SII] and H alpha frames) and of the aligned knots within ~30" from the outflow source (only from the [SII] frames). We find that the present-day motions of the knots along the HH 34 jet are approximately ballistic, and that these motions directly imply the formation of a major mass concentration in ~900 yr, at a position similar to the one of the present-day HH 34S bow shock. In other words, we find that the knots along the HH 34 jet will merge to form a more massive structure, possibly resembling HH 34S.
doi_str_mv 10.1088/0004-637X/748/2/103
format Article
fullrecord <record><control><sourceid>proquest_osti_</sourceid><recordid>TN_cdi_osti_scitechconnect_22016104</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>1680447672</sourcerecordid><originalsourceid>FETCH-LOGICAL-c303t-a9042c68bff2de737ba6d62e5da639357c239ad5249d4e337101d061a2bb96c83</originalsourceid><addsrcrecordid>eNqNkV1LwzAUhoMoOKe_wJuACN7UJTlp0l7W0a3FfcBWUa9ClqZY2dbZdBf-ezM2du3V4bw857znA6F7Sp4piaIBIYQHAuTHQPJowAaUwAXq0RCigEMoL1HvTFyjG-e-DymL4x4aFVmKX_NZOk2KfLjE8xHOMgwcjxbzKc6WBc6nyThd4ve8yHCCZx4NPtNkgYt8muKXZJlOvHSLriq9dvbuFPvobZQWwyyYzMf5MJkEBgh0gY69rRHRqqpYaSXIlRalYDYstYDYT2oYxLoMGY9LbgEkJbQkgmq2WsXCRNBHD8e-jetq5UzdWfNlmu3Wmk4xRqighHvq6Ujt2uZnb12nNrUzdr3WW9vsnaIiCiMAzuh_UMK5FJJ5FI6oaRvnWlupXVtvdPurKFGHN6jDVdXhyMq_QTEvgq96PBloZ_S6avXW1O5cygTzy1IJf02zfdY</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>1680447672</pqid></control><display><type>article</type><title>THE KINEMATICS OF HH 34 FROM HST IMAGES WITH A NINE-YEAR TIME BASELINE</title><source>Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals</source><source>Institute of Physics Open Access Journal Titles</source><source>Alma/SFX Local Collection</source><creator>RAGA, A. C ; NORIEGA-CRESPO, A ; RODRIGUEZ-GONZALEZ, A ; LORA, V ; STAPELFELDT, K. R ; CAREY, S. J</creator><creatorcontrib>RAGA, A. C ; NORIEGA-CRESPO, A ; RODRIGUEZ-GONZALEZ, A ; LORA, V ; STAPELFELDT, K. R ; CAREY, S. J</creatorcontrib><description>We study archival HST [SII] 6716+30 and H alpha images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The ~9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the HH 34S bow shock (from the [SII] and H alpha frames) and of the aligned knots within ~30" from the outflow source (only from the [SII] frames). We find that the present-day motions of the knots along the HH 34 jet are approximately ballistic, and that these motions directly imply the formation of a major mass concentration in ~900 yr, at a position similar to the one of the present-day HH 34S bow shock. In other words, we find that the knots along the HH 34 jet will merge to form a more massive structure, possibly resembling HH 34S.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.1088/0004-637X/748/2/103</identifier><identifier>CODEN: ASJOAB</identifier><language>eng</language><publisher>Bristol: IOP</publisher><subject>Alignment ; Angular resolution ; Astronomy ; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ; Earth, ocean, space ; Exact sciences and technology ; Formations ; Frames ; HERBIG-HARO OBJECTS ; INTERSTELLAR GRAINS ; Kinematics ; Knots ; MASS ; Outflow ; PROPER MOTION ; SHOCK WAVES ; STARS ; Substructures</subject><ispartof>The Astrophysical journal, 2012-04, Vol.748 (2), p.1-10</ispartof><rights>2015 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c303t-a9042c68bff2de737ba6d62e5da639357c239ad5249d4e337101d061a2bb96c83</citedby><cites>FETCH-LOGICAL-c303t-a9042c68bff2de737ba6d62e5da639357c239ad5249d4e337101d061a2bb96c83</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,778,782,883,27907,27908</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=26224917$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/22016104$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>RAGA, A. C</creatorcontrib><creatorcontrib>NORIEGA-CRESPO, A</creatorcontrib><creatorcontrib>RODRIGUEZ-GONZALEZ, A</creatorcontrib><creatorcontrib>LORA, V</creatorcontrib><creatorcontrib>STAPELFELDT, K. R</creatorcontrib><creatorcontrib>CAREY, S. J</creatorcontrib><title>THE KINEMATICS OF HH 34 FROM HST IMAGES WITH A NINE-YEAR TIME BASELINE</title><title>The Astrophysical journal</title><description>We study archival HST [SII] 6716+30 and H alpha images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The ~9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the HH 34S bow shock (from the [SII] and H alpha frames) and of the aligned knots within ~30" from the outflow source (only from the [SII] frames). We find that the present-day motions of the knots along the HH 34 jet are approximately ballistic, and that these motions directly imply the formation of a major mass concentration in ~900 yr, at a position similar to the one of the present-day HH 34S bow shock. In other words, we find that the knots along the HH 34 jet will merge to form a more massive structure, possibly resembling HH 34S.</description><subject>Alignment</subject><subject>Angular resolution</subject><subject>Astronomy</subject><subject>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Formations</subject><subject>Frames</subject><subject>HERBIG-HARO OBJECTS</subject><subject>INTERSTELLAR GRAINS</subject><subject>Kinematics</subject><subject>Knots</subject><subject>MASS</subject><subject>Outflow</subject><subject>PROPER MOTION</subject><subject>SHOCK WAVES</subject><subject>STARS</subject><subject>Substructures</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqNkV1LwzAUhoMoOKe_wJuACN7UJTlp0l7W0a3FfcBWUa9ClqZY2dbZdBf-ezM2du3V4bw857znA6F7Sp4piaIBIYQHAuTHQPJowAaUwAXq0RCigEMoL1HvTFyjG-e-DymL4x4aFVmKX_NZOk2KfLjE8xHOMgwcjxbzKc6WBc6nyThd4ve8yHCCZx4NPtNkgYt8muKXZJlOvHSLriq9dvbuFPvobZQWwyyYzMf5MJkEBgh0gY69rRHRqqpYaSXIlRalYDYstYDYT2oYxLoMGY9LbgEkJbQkgmq2WsXCRNBHD8e-jetq5UzdWfNlmu3Wmk4xRqighHvq6Ujt2uZnb12nNrUzdr3WW9vsnaIiCiMAzuh_UMK5FJJ5FI6oaRvnWlupXVtvdPurKFGHN6jDVdXhyMq_QTEvgq96PBloZ_S6avXW1O5cygTzy1IJf02zfdY</recordid><startdate>20120401</startdate><enddate>20120401</enddate><creator>RAGA, A. C</creator><creator>NORIEGA-CRESPO, A</creator><creator>RODRIGUEZ-GONZALEZ, A</creator><creator>LORA, V</creator><creator>STAPELFELDT, K. R</creator><creator>CAREY, S. J</creator><general>IOP</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>OTOTI</scope></search><sort><creationdate>20120401</creationdate><title>THE KINEMATICS OF HH 34 FROM HST IMAGES WITH A NINE-YEAR TIME BASELINE</title><author>RAGA, A. C ; NORIEGA-CRESPO, A ; RODRIGUEZ-GONZALEZ, A ; LORA, V ; STAPELFELDT, K. R ; CAREY, S. J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c303t-a9042c68bff2de737ba6d62e5da639357c239ad5249d4e337101d061a2bb96c83</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Alignment</topic><topic>Angular resolution</topic><topic>Astronomy</topic><topic>ASTROPHYSICS, COSMOLOGY AND ASTRONOMY</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Formations</topic><topic>Frames</topic><topic>HERBIG-HARO OBJECTS</topic><topic>INTERSTELLAR GRAINS</topic><topic>Kinematics</topic><topic>Knots</topic><topic>MASS</topic><topic>Outflow</topic><topic>PROPER MOTION</topic><topic>SHOCK WAVES</topic><topic>STARS</topic><topic>Substructures</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>RAGA, A. C</creatorcontrib><creatorcontrib>NORIEGA-CRESPO, A</creatorcontrib><creatorcontrib>RODRIGUEZ-GONZALEZ, A</creatorcontrib><creatorcontrib>LORA, V</creatorcontrib><creatorcontrib>STAPELFELDT, K. R</creatorcontrib><creatorcontrib>CAREY, S. J</creatorcontrib><collection>Pascal-Francis</collection><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>OSTI.GOV</collection><jtitle>The Astrophysical journal</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>RAGA, A. C</au><au>NORIEGA-CRESPO, A</au><au>RODRIGUEZ-GONZALEZ, A</au><au>LORA, V</au><au>STAPELFELDT, K. R</au><au>CAREY, S. J</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>THE KINEMATICS OF HH 34 FROM HST IMAGES WITH A NINE-YEAR TIME BASELINE</atitle><jtitle>The Astrophysical journal</jtitle><date>2012-04-01</date><risdate>2012</risdate><volume>748</volume><issue>2</issue><spage>1</spage><epage>10</epage><pages>1-10</pages><issn>0004-637X</issn><eissn>1538-4357</eissn><coden>ASJOAB</coden><abstract>We study archival HST [SII] 6716+30 and H alpha images of the HH 34 outflow, taken in 1998.71 and in 2007.83. The ~9 yr time baseline and the high angular resolution of these observations allow us to carry out a detailed proper-motion study. We determine the proper motions of the substructure of the HH 34S bow shock (from the [SII] and H alpha frames) and of the aligned knots within ~30" from the outflow source (only from the [SII] frames). We find that the present-day motions of the knots along the HH 34 jet are approximately ballistic, and that these motions directly imply the formation of a major mass concentration in ~900 yr, at a position similar to the one of the present-day HH 34S bow shock. In other words, we find that the knots along the HH 34 jet will merge to form a more massive structure, possibly resembling HH 34S.</abstract><cop>Bristol</cop><pub>IOP</pub><doi>10.1088/0004-637X/748/2/103</doi><tpages>10</tpages></addata></record>
fulltext fulltext
identifier ISSN: 0004-637X
ispartof The Astrophysical journal, 2012-04, Vol.748 (2), p.1-10
issn 0004-637X
1538-4357
language eng
recordid cdi_osti_scitechconnect_22016104
source Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Institute of Physics Open Access Journal Titles; Alma/SFX Local Collection
subjects Alignment
Angular resolution
Astronomy
ASTROPHYSICS, COSMOLOGY AND ASTRONOMY
Earth, ocean, space
Exact sciences and technology
Formations
Frames
HERBIG-HARO OBJECTS
INTERSTELLAR GRAINS
Kinematics
Knots
MASS
Outflow
PROPER MOTION
SHOCK WAVES
STARS
Substructures
title THE KINEMATICS OF HH 34 FROM HST IMAGES WITH A NINE-YEAR TIME BASELINE
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-16T17%3A10%3A32IST&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%20KINEMATICS%20OF%20HH%2034%20FROM%20HST%20IMAGES%20WITH%20A%20NINE-YEAR%20TIME%20BASELINE&rft.jtitle=The%20Astrophysical%20journal&rft.au=RAGA,%20A.%20C&rft.date=2012-04-01&rft.volume=748&rft.issue=2&rft.spage=1&rft.epage=10&rft.pages=1-10&rft.issn=0004-637X&rft.eissn=1538-4357&rft.coden=ASJOAB&rft_id=info:doi/10.1088/0004-637X/748/2/103&rft_dat=%3Cproquest_osti_%3E1680447672%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=1680447672&rft_id=info:pmid/&rfr_iscdi=true