Hādhihi Ḥāshiyat al-ʻālim al-himām wa-al-ʻallāmah al-Imām al-Shaykh Ibrāhīm al-Bājūrī ʻalá matn al-Shamāʼil al-Muḥammadīyah ʻalá ṣāḥibihā afḍal al-ṣalāh wa-azká al-taḥīyah lil-Imām al-muḥaqqiq wa-al-muḥaddith al-mudaqqiq Muḥammad ibn ʻĪsá al-Tirmidhī.

Mode of access: Internet.

Hādhā kitāb Tarkīb Khālid wa-bi-hi nastaʻīn [microform]

Microfilm.

Hādhā Dīwān al-ḥaqāʼiq wa-majmūʻ al-raqāʼiq fī ṣarīḥ al-mawājīd al-Ilāhīyah wa-al-tajallīyāt al-rabbānīyah wa-al-futūḥāt al-aqdasīyah wa-huwa al-bāb al-awwal min Dīwān al-dawāwīn wa-rayḥān al-rayāḥīn fī tajallīyat al-ḥaqq al-mubīn ʻalá jamīʻ anwāʻ al-ṣiyagh wa-al-talāwīn [microform] /

Microfilm.

Sharḥ al-Manār wa-ḥawāshīhi min ʻilm al-uṣūl [microform] /

On the margins: Glosses by ʻAzmīźādah and Ibn al-Ḥanbalī.

Ofel Bat-Tsiyon : maśa ḥizayon be-arbaʻa maḥazot. Ḳinah hi ʻal mot meshorer shire Bat-Tsiyon.

Mode of access: Internet.

Ḳiryah niʹsgavah : hi ha-ʻir Zolḳoṿa, rabanehah, geʾonehah, ḥakhamehah, parnasehah u-manhigehah, shemot ha-sefarim asher ḥubru ... /

"# aus der Vlerteljahresschrift 'Haeschkol.'"

Śefat yeter : ... le-hatsil Rabenu Saʻadyah gaʾon ... min ha-haśagot she-hiśig ʻalav ... Donash ben Lavraṭ ... /

Title on added t.p.: Sephet Jether.

Kitāb-i muqaddas kā pahlā hiṣṣah yaʻnī purānā ʻahd nāmah = Old Testament in Urdu : with references.

Mode of access: Internet.

Lexici Euripidei : specimen novum quo continentur literae H vocabula : h-hiōn /

"1891. Gymn. Wismar. Progr. No. 647."

Ḥeshbon ha-nefesh : hi taḥbulah niflaʾah le-hitrapʾut maḥale ha-midot ʻal yede hatmadat ḥinukh tiḳunehen... /

Photographic reproduction of the copy in the Hebrew Union College Library, Cincinnati, Ohio.

"Hi-ya, neighbor,"

"Intimate glimpses of Franklin D. Roosevelt at Warm Springs, Georgia."

Hādhā Kitāb jāmiʻ al-mutūn fī ḥaqq anwāʻ al-ṣifāt al-ilāhīyah wa-al-ʻaqāʼid al-Māturīdīyah wa-alfāẓ al-kufr wa-taṣḥīḥ al-aʻmāl al-ʻajībīyah [microform] /

Microfilm.

Ḥāshiyat ... Ibrāhīm al-Bājūrī al-musammāh bi-al-Mawāhib al-ladunīyah ʻalá al-Shamāʼil al-Muḥammadīyah [microform] /

Caption title.

ATCA HI observations of the peculiar galaxy IC 2554

ATCA H I and radio continuum observations of the peculiar southern galaxy IC 2554 and its surroundings reveal typical signatures of an interacting galaxy group. We detected a large H I cloud between IC 2554 and the elliptical galaxy NGC 3136B. The gas dynamics in IC 2554 itself, which is sometimes described as a colliding pair, are surprisingly regular, whereas NGC 3136B was not detected. The H I cloud, which emerges from IC 2554 as a large arc-shaped plume, has a size of similar to30 kpc, larger than that of IC 2554. The total H I mass of the IC 2554 system is similar to2 x 10(9) M., one-third of which resides in the H I cloud. It is possible that tidal interaction between IC 2554 and NGC 3136B caused this spectacular H I cloud, but the possibility of IC 2554 being a merger remnant is also discussed. We also detected H I gas in the nearby galaxies ESO 092-G009 and RKK 1959 and an associated H I cloud, ATCA J1006-6710. Together they have an H I mass of similar to4.6 x 10(8) M-.. Another new H I source, ATCA J1007-6659, with an H I mass of only similar to2.2 x 10(7) M. was detected roughly between IC 2554 and ESO 092-G009 and corresponds to a face-on low surface brightness dwarf galaxy. Star formation is evident only in the galaxy IC 2554 with a rate of similar to4 M. yr(-1).

The Hi content of compact groups of galaxies

The Hi content of Hickson Compact Groups in the southern hemisphere is measured using data from the Hi Parkes All-Sky Survey (HIPASS), and dedicated observations using the narrow band filter on the Multibeam instrument on the Parkes telescope. The expected Hi mass of these groups was estimated using the luminosity, diameter, and morphological types of the member galaxies, calibrated from published data. Taking careful account of non-detection limits, the results show that the compact group population that has been detected by these observations has an Hi content similar to that of galaxies in the reference field sample. The upper limits for the undetected groups lie within the normal range; improvement of these limits will require a large increase in sensitivity.