Loading…

Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star

We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of...

Full description

Saved in:
Bibliographic Details
Published in:Publications of the Astronomical Society of the Pacific 1993-06, Vol.105 (688), p.599-602
Main Authors: Kaler, James B., Bell, David, Hayes, John, Stanghellini, Letizia
Format: Article
Language:English
Subjects:
Citations: Items that cite this one
Online Access:Get full text
Tags: Add Tag
No Tags, Be the first to tag this record!
cited_by cdi_FETCH-LOGICAL-c236t-72b9f0b49d1f48cce87f35c82737f1ba554c67ebd860f577d9fe27bfb35455313
cites
container_end_page 602
container_issue 688
container_start_page 599
container_title Publications of the Astronomical Society of the Pacific
container_volume 105
creator Kaler, James B.
Bell, David
Hayes, John
Stanghellini, Letizia
description We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of a symbiotic star.
doi_str_mv 10.1086/133202
format article
fullrecord <record><control><sourceid>jstor_cross</sourceid><recordid>TN_cdi_crossref_primary_10_1086_133202</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><jstor_id>40680078</jstor_id><sourcerecordid>40680078</sourcerecordid><originalsourceid>FETCH-LOGICAL-c236t-72b9f0b49d1f48cce87f35c82737f1ba554c67ebd860f577d9fe27bfb35455313</originalsourceid><addsrcrecordid>eNpF0MFKxDAQBuAgCtZV30DIQbxVJ0nTpEdZdBUWXaieS5Im2KVtShIP-_Z2qehpGOZjmH8QuiZwT0CWD4QxCvQEZYQzmTMp2CnKAKDISyrhHF3EuAcgRBLI0KaerEnBT18--cGmcMDeYcLxrlejTWru36z-7pXFamyxwjsfY6d7i-vDoDufOoPrmV2iM6f6aK9-6wp9Pj99rF_y7fvmdf24zQ1lZcoF1ZUDXVQtcYU0xkrhGDeSCiYc0YrzwpTC6laW4LgQbeUsFdppxgvOGWErdLfsNWE-JFjXTKEb5jMbAs0xfrPEn-HtAicVjepdUKPp4p8u5PEBfGY3C9vH5MP_GEoJICT7AchTYbg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star</title><source>JSTOR Archival Journals and Primary Sources Collection</source><source>Institute of Physics</source><creator>Kaler, James B. ; Bell, David ; Hayes, John ; Stanghellini, Letizia</creator><creatorcontrib>Kaler, James B. ; Bell, David ; Hayes, John ; Stanghellini, Letizia</creatorcontrib><description>We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of a symbiotic star.</description><identifier>ISSN: 0004-6280</identifier><identifier>EISSN: 1538-3873</identifier><identifier>DOI: 10.1086/133202</identifier><identifier>CODEN: PASPAU</identifier><language>eng</language><publisher>Chicago, IL: American Institute of Physics</publisher><subject>Astronomical objects ; Astronomy ; Density ; Earth, ocean, space ; Exact sciences and technology ; Helium ; Interstellar extinction ; Interstellar medium (ism) and nebulae in milky way ; Nebulae ; Nitrogen ; Planetary nebulae ; Stars ; Stellar spectra ; Stellar systems. Galactic and extragalactic objects and systems. The universe ; Symbiotic stars</subject><ispartof>Publications of the Astronomical Society of the Pacific, 1993-06, Vol.105 (688), p.599-602</ispartof><rights>1993 INIST-CNRS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c236t-72b9f0b49d1f48cce87f35c82737f1ba554c67ebd860f577d9fe27bfb35455313</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/40680078$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/40680078$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,778,782,27911,27912,58225,58458</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&amp;idt=4811815$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Kaler, James B.</creatorcontrib><creatorcontrib>Bell, David</creatorcontrib><creatorcontrib>Hayes, John</creatorcontrib><creatorcontrib>Stanghellini, Letizia</creatorcontrib><title>Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star</title><title>Publications of the Astronomical Society of the Pacific</title><description>We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of a symbiotic star.</description><subject>Astronomical objects</subject><subject>Astronomy</subject><subject>Density</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Helium</subject><subject>Interstellar extinction</subject><subject>Interstellar medium (ism) and nebulae in milky way</subject><subject>Nebulae</subject><subject>Nitrogen</subject><subject>Planetary nebulae</subject><subject>Stars</subject><subject>Stellar spectra</subject><subject>Stellar systems. Galactic and extragalactic objects and systems. The universe</subject><subject>Symbiotic stars</subject><issn>0004-6280</issn><issn>1538-3873</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1993</creationdate><recordtype>article</recordtype><recordid>eNpF0MFKxDAQBuAgCtZV30DIQbxVJ0nTpEdZdBUWXaieS5Im2KVtShIP-_Z2qehpGOZjmH8QuiZwT0CWD4QxCvQEZYQzmTMp2CnKAKDISyrhHF3EuAcgRBLI0KaerEnBT18--cGmcMDeYcLxrlejTWru36z-7pXFamyxwjsfY6d7i-vDoDufOoPrmV2iM6f6aK9-6wp9Pj99rF_y7fvmdf24zQ1lZcoF1ZUDXVQtcYU0xkrhGDeSCiYc0YrzwpTC6laW4LgQbeUsFdppxgvOGWErdLfsNWE-JFjXTKEb5jMbAs0xfrPEn-HtAicVjepdUKPp4p8u5PEBfGY3C9vH5MP_GEoJICT7AchTYbg</recordid><startdate>19930601</startdate><enddate>19930601</enddate><creator>Kaler, James B.</creator><creator>Bell, David</creator><creator>Hayes, John</creator><creator>Stanghellini, Letizia</creator><general>American Institute of Physics</general><general>University of Chicago Press</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>19930601</creationdate><title>Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star</title><author>Kaler, James B. ; Bell, David ; Hayes, John ; Stanghellini, Letizia</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c236t-72b9f0b49d1f48cce87f35c82737f1ba554c67ebd860f577d9fe27bfb35455313</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1993</creationdate><topic>Astronomical objects</topic><topic>Astronomy</topic><topic>Density</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Helium</topic><topic>Interstellar extinction</topic><topic>Interstellar medium (ism) and nebulae in milky way</topic><topic>Nebulae</topic><topic>Nitrogen</topic><topic>Planetary nebulae</topic><topic>Stars</topic><topic>Stellar spectra</topic><topic>Stellar systems. Galactic and extragalactic objects and systems. The universe</topic><topic>Symbiotic stars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Kaler, James B.</creatorcontrib><creatorcontrib>Bell, David</creatorcontrib><creatorcontrib>Hayes, John</creatorcontrib><creatorcontrib>Stanghellini, Letizia</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><jtitle>Publications of the Astronomical Society of the Pacific</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Kaler, James B.</au><au>Bell, David</au><au>Hayes, John</au><au>Stanghellini, Letizia</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star</atitle><jtitle>Publications of the Astronomical Society of the Pacific</jtitle><date>1993-06-01</date><risdate>1993</risdate><volume>105</volume><issue>688</issue><spage>599</spage><epage>602</epage><pages>599-602</pages><issn>0004-6280</issn><eissn>1538-3873</eissn><coden>PASPAU</coden><abstract>We provide line intensities and limited chemical compositions of a collection of planetary nebulae, most of which are within 25° of the Galactic center. Several appear enriched in nitrogen and/or helium. The central star of M1-51 displays C iv in emission. Ha 1-2 has the spectral characteristics of a symbiotic star.</abstract><cop>Chicago, IL</cop><pub>American Institute of Physics</pub><doi>10.1086/133202</doi><tpages>4</tpages><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier ISSN: 0004-6280
ispartof Publications of the Astronomical Society of the Pacific, 1993-06, Vol.105 (688), p.599-602
issn 0004-6280
1538-3873
language eng
recordid cdi_crossref_primary_10_1086_133202
source JSTOR Archival Journals and Primary Sources Collection; Institute of Physics
subjects Astronomical objects
Astronomy
Density
Earth, ocean, space
Exact sciences and technology
Helium
Interstellar extinction
Interstellar medium (ism) and nebulae in milky way
Nebulae
Nitrogen
Planetary nebulae
Stars
Stellar spectra
Stellar systems. Galactic and extragalactic objects and systems. The universe
Symbiotic stars
title Spectrophotometry of 15 Planetary Nebulae and a Possible Symbiotic Star
url http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-15T17%3A19%3A32IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-jstor_cross&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Spectrophotometry%20of%2015%20Planetary%20Nebulae%20and%20a%20Possible%20Symbiotic%20Star&rft.jtitle=Publications%20of%20the%20Astronomical%20Society%20of%20the%20Pacific&rft.au=Kaler,%20James%20B.&rft.date=1993-06-01&rft.volume=105&rft.issue=688&rft.spage=599&rft.epage=602&rft.pages=599-602&rft.issn=0004-6280&rft.eissn=1538-3873&rft.coden=PASPAU&rft_id=info:doi/10.1086/133202&rft_dat=%3Cjstor_cross%3E40680078%3C/jstor_cross%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-c236t-72b9f0b49d1f48cce87f35c82737f1ba554c67ebd860f577d9fe27bfb35455313%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rft_jstor_id=40680078&rfr_iscdi=true